Relevant bibliographies by topics / Stars: individual: BY Cam

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  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers
  6. Reports

Academic literature on the topic 'Stars: individual: BY Cam'

Author: Grafiati
Published: 4 June 2021
Last updated: 12 February 2022

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Journal articles on the topic "Stars: individual: BY Cam"

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Topasna, G. A., N. T. Kaltcheva, and E. Paunzen. "Interstellar polarization and extinction towards the young open cluster NGC 1502." Astronomy & Astrophysics 615 (July 2018): A166. http://dx.doi.org/10.1051/0004-6361/201731903.

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Aims. NGC 1502 is located at the periphery of the Cam OB1 association and probably within the Orion Spur, with published distance estimates varying between 0.7 and 1.5 kpc. We combine new polarimetric observations and existing uvbyβ and UBV photometries to provide new estimates of the cluster’s parameters. Methods. We present new multi-wavelength polarization observations of 22 stars in the direction of the cluster and, using the wavelength of maximum polarization, calculate the total-to-selective extinction ratio for each of these stars. These are combined with homogenized uvbyβ and UBV photo
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Schechter, Paul L., Jeffrey A. Blackburne, David Pooley, and Joachim Wambsganss. "Stellar masses calibrated with micro-lensed quasars." Proceedings of the International Astronomical Union 10, S311 (2014): 96–99. http://dx.doi.org/10.1017/s1743921315003464.

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AbstractWe measure the stellar mass surface densities of early type galaxies by observing the micro-lensing of macro-lensed quasars caused by individual stars, including stellar remnants, brown dwarfs and red dwarfs too faint to produce photometric or spectroscopic signatures. Our method measures the graininess of the gravitational potential, in contrast to methods that decompose a smooth total gravitational potential into two smooth components, one stellar and one dark. We find the median likelihood value for the calibration factor $\cal F$ by which Salpeter stellar masses (with a low mass cu
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Mosler, Andrea B., Adam Weir, Andreas Serner, et al. "Musculoskeletal Screening Tests and Bony Hip Morphology Cannot Identify Male Professional Soccer Players at Risk of Groin Injuries: A 2-Year Prospective Cohort Study." American Journal of Sports Medicine 46, no. 6 (2018): 1294–305. http://dx.doi.org/10.1177/0363546518763373.

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Background: Musculoskeletal hip/groin screening tests are commonly performed to detect at-risk individuals. Bony hip morphology is considered a potential intrinsic risk factor but has not been examined prospectively. Purpose: To evaluate the association between intrinsic risk factors identified from musculoskeletal and radiographic screening tests and hip/groin injuries leading to time loss from training and/or match play in professional male soccer players. Study Design: Prospective cohort study; Level of evidence, 2. Methods: Male professional soccer players, aged ≥18 years, underwent screen
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Babel, J. "Diffusion Models for Magnetic Ap Stars." International Astronomical Union Colloquium 138 (1993): 458–72. http://dx.doi.org/10.1017/s025292110002090x.

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AbstractProgress made in spectroscopy and in the diffusion theory permits now to make severe comparisons, based on line profiles, between theory and observation.We first review transport processes which are present in the atmospheric layers of Ap stars and discuss their relative importance. We then show that mass loss could play a key role for the creation of abundance maps. A mass loss model is proposed for 53 Cam and is compared, by spectrum synthesis, with visible and IUE high resolutions observations. The model accounts well for the line profiles of several elements with an exception for T
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Raveendran, A. V., N. Kameswara Rao, M. R. Deshpande, U. C. Joshi, and A. K. Kulshrestha. "Polarimetric Observations of Hydrogen Deficient Stars." International Astronomical Union Colloquium 87 (1985): 167–71. http://dx.doi.org/10.1017/s0252921100090710.

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AbstractPolarimetric observations of HD 30353, SU Tau, XX Cam, R Cr B,UV Cas, BD+13 3224,BD+10 2179 and HD 124448 are presented. The linear polarization of HD 30353 is found to vary appreciably at Hα over time scale as short as one day. It is also found that SU Tau shows significant variation in polarisation even at light maximum.
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Williams, R. K., C. Goridis, and R. Akeson. "Individual neural cell types express immunologically distinct N-CAM forms." Journal of Cell Biology 101, no. 1 (1985): 36–42. http://dx.doi.org/10.1083/jcb.101.1.36.

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The neural cell adhesion molecules, or N-CAMs, are a group of structurally and immunologically related glycoproteins found in vertebrate neural tissues. Adult brain N-CAMs have apparent molecular weights of 180,000, 140,000, and 120,000. In this article we identify, using monoclonal antibody (Mab) 3G6.41, an immunologically distinct adult rat N-CAM form and show that this form is selectively expressed by some clonal neural cell lines. Consecutive immunoprecipitation experiments indicate that rabbit anti-N-CAM can remove from solubilized cerebellar neuron primary cultures all 180,000- and 140,0
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Buat-Ménard, V., J. M. Hameury, and J. P. Lasota. "Z Cam stars: A particular response to a general phenomenon." Astronomy & Astrophysics 369, no. 3 (2001): 925–31. http://dx.doi.org/10.1051/0004-6361:20010176.

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Hameury, J. M., and J. P. Lasota. "Anomalous Z Cam stars: a response to mass-transfer outbursts." Astronomy & Astrophysics 569 (September 2014): A48. http://dx.doi.org/10.1051/0004-6361/201424535.

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Babel, J. "A Diffusion Mass-Loss Model for the Ap Star 53 Cam." International Astronomical Union Colloquium 137 (1993): 275–77. http://dx.doi.org/10.1017/s0252921100017905.

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AbstractThe mechanism and properties of mass loss are poorly known for Ap stars. Present upper limits on the mass loss rate are of 10−10 M⊙yr−1, a value which does not permit any element separation. Abundance maps could be a very powerful tool to constrain the mass loss rate and the wind geometry of Ap stars, as surface abundances are sensitive to rates as small as 10−15 M⊙yr−1. We here propose a diffusion-mass loss model for 53 Cam and compute abundance distributions in the photosphere of 53 Cam. The mass loss geometry is determined from the Ca II K line profile and its time variation. We obt
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Halling, D. Brent, Benjamin J. Liebeskind, Amelia W. Hall, and Richard W. Aldrich. "Conserved properties of individual Ca2+-binding sites in calmodulin." Proceedings of the National Academy of Sciences 113, no. 9 (2016): E1216—E1225. http://dx.doi.org/10.1073/pnas.1600385113.

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Calmodulin (CaM) is a Ca2+-sensing protein that is highly conserved and ubiquitous in eukaryotes. In humans it is a locus of life-threatening cardiomyopathies. The primary function of CaM is to transduce Ca2+ concentration into cellular signals by binding to a wide range of target proteins in a Ca2+-dependent manner. We do not fully understand how CaM performs its role as a high-fidelity signal transducer for more than 300 target proteins, but diversity among its four Ca2+-binding sites, called EF-hands, may contribute to CaM’s functional versatility. We therefore looked at the conservation of
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Dissertations / Theses on the topic "Stars: individual: BY Cam"

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Tutar, Özdarcan D., P. S. Smith, and V. Keskin. "Time-resolved spectropolarimetric observations of polars WX LMi and BY Cam." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/624423.

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Time-series spectropolarimetric observations of polar WX LMi and asynchronous polar BY Cam are presented. Magnetic field properties, radial velocities and optical polarization are investigated via consecutive observations with good phase sampling during a single orbital cycle. Both systems are found to have a decentred dipole magnetic field configuration. One of the poles of WX LMi has a field strength of 49 MG, while the other pole may have possible field strengths of 69, 104 or 207 MG, depending on the harmonic numbers of the cyclotron humps observed in the circularly polarized spectrum. For
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Spruyt, Jon. "Gamified Individual Brainstorming : Reaching for the stars." Thesis, Umeå universitet, Institutionen för informatik, 2017. http://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-133603.

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Ideation is a critical step in the creation of new solutions to problems. Brainstorming, being the most commonly known ideation method, is mostly done in groups. However, research points out that brainstorming individually is more effective than brainstorming in groups. This paper investigates if negative aspects (reduced enjoyment, motivation and self-rated performance) associated with brainstorming alone can be overcome by using a gamified approach to brainstorming. Gamified and non-gamified prototypes have been made and used in combination with a questionnaire to measure differences in thes
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Fossati, L., T. Koskinen, K. France, et al. "Suppressed Far-UV Stellar Activity and Low Planetary Mass Loss in the WASP-18 System." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627089.

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WASP-18 hosts a massive, very close-in Jupiter-like planet. Despite its young age (< 1 Gyr), the star presents an anomalously low stellar activity level: the measured log R'(HK) activity parameter lies slightly below the basal level; there is no significant time-variability in the log R'(HK) value; there is no detection of the star in the X-rays. We present results of far-UV observations of WASP-18 obtained with COS on board of Hubble Space Telescope aimed at explaining this anomaly. From the star's spectral energy distribution, we infer the extinction (E(B-V) approximate to 0.01 mag) and then
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Brunsden, Emily. "The Music of the Stars : Spectroscopy of Pulsations in gamma Doradus Stars." Thesis, University of Canterbury. Astronomy, 2013. http://hdl.handle.net/10092/8373.

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The mysteries of the interior structures of stars are being tackled with asteroseismology. The observable parameters of the surface pulsations of stars inform us of the interior characteristics of numerous classes of stars. The main-sequence gamma Doradus stars, just a little hotter than the Sun, offer the potential of determining stellar structure right down to the core. To determine the structural profile of a star, the observed frequencies and a full geometric description must be determined. This is only possible with long-term spectroscopic monitoring and careful analysis of the pulsation
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Boyajian, Tabetha S., Roi Alonso, Alex Ammerman, et al. "The First Post-Kepler Brightness Dips of KIC 8462852." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/626540.

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We present a photometric detection of the first brightness dips of the unique variable star KIC 8462852 since the end of the Kepler space mission in 2013 May. Our regular photometric surveillance started in 2015 October, and a sequence of dipping began in 2017 May continuing on through the end of 2017, when the star was no longer visible from Earth. We distinguish four main 1%-2.5% dips, named "Elsie," "Celeste," "Skara Brae," and " Angkor," which persist on timescales from several days to weeks. Our main results so far are as follows: (i) there are no apparent changes of the stellar spectrum
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Lew, Ben W. P., Daniel Apai, Yifan Zhou, et al. "CLOUD ATLAS: DISCOVERY OF PATCHY CLOUDS AND HIGH-AMPLITUDE ROTATIONAL MODULATIONS IN A YOUNG, EXTREMELY RED L-TYPE BROWN DWARF." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622769.

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Condensate clouds fundamentally impact the atmospheric structure and spectra of exoplanets and brown dwarfs, but the connections between surface gravity, cloud structure, dust in the upper atmosphere, and the red colors of some brown dwarfs remain poorly understood. Rotational modulations enable the study of different clouds in the same atmosphere, thereby providing a method to isolate the effects of clouds. Here, we present the discovery of high peak-to-peak amplitude (8%) rotational modulations in a low-gravity, extremely red (J-K-s = 2.55) L6 dwarf WISEP J004701.06+680352.1 (W0047). Using t
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Kiminki, Megan M., Megan Reiter та Nathan Smith. "Ancient eruptions of η Carinae: a tale written in proper motions". OXFORD UNIV PRESS, 2016. http://hdl.handle.net/10150/622109.

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We analyse eight epochs of Hubble Space Telescope H alpha+[N ii] imaging of eta Carinae's outer ejecta. Proper motions of nearly 800 knots reveal that the detected ejecta are divided into three apparent age groups, dating to around 1250 A.D., to around 1550 A.D., and to during or shortly before the Great Eruption of the 1840s. Ejecta from these groups reside in different locations and provide a firm constraint that eta Car experienced multiple major eruptions prior to the nineteenth century. The 1250 and 1550 events did not share the same axisymmetry as the Homunculus; the 1250 event was parti
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Currie, Thayne, Olivier Guyon, Motohide Tamura, et al. "Subaru/SCExAO First-light Direct Imaging of a Young Debris Disk around HD 36546." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624379.

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We present H-band scattered light imaging of a bright debris disk around the A0 star HD 36546 obtained from the Subaru Coronagraphic Extreme Adaptive Optics (SCExAO) system with data recorded by the HiCIAO camera using the vector vortex coronagraph. SCExAO traces the disk from r similar to 0."3 to r similar to 1" (34-114 au). The disk is oriented in a near east-west direction (PA similar to 75 degrees), is inclined by i similar to 70 degrees-75 degrees, and is strongly forward-scattering (g > 0.5). It is an extended disk rather than a sharp ring; a second, diffuse dust population extends from
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Wu, Ya-Lin, Nathan Smith, Laird M. Close, Jared R. Males, and Katie M. Morzinski. "Resolving the H alpha-emitting Region in the Wind of eta Carinae." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624482.

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The massive evolved star. Carinae is the most luminous star in the Milky Way and has the highest steady wind mass-loss rate of any known star. Radiative transfer models of the spectrum by Hillier et al. predict that Ha is mostly emitted in regions of the wind at radii of 6-60 au from the star (2.5-25 mas at 2.35 kpc). We present diffraction-limited images (FWHM similar to 25 mas) with Magellan adaptive optics in two epochs, showing that. Carinae consistently appears similar to 2.5-3 mas wider in Ha emission compared to the adjacent 643 nm continuum. This implies that the H alpha line-forming r
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Hełminiak, K. G., M. Kuzuhara, K. Mede, et al. "SEEDS DIRECT IMAGING OF THE RV-DETECTED COMPANION TO V450 ANDROMEDAE, AND CHARACTERIZATION OF THE SYSTEM." IOP PUBLISHING LTD, 2016. http://hdl.handle.net/10150/622454.

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We report the direct imaging detection of a low-mass companion to a young, moderately active star V450. And, that was previously identified with the radial velocity (RV) method. The companion was found in high-contrast images obtained with the Subaru Telescope equipped with the HiCIAO camera and AO188 adaptive optics system. From the public ELODIE and SOPHIE archives we extracted available high-resolution spectra and RV measurements, along with RVs from the Lick planet search program. We combined our multi-epoch astrometry with these archival, partially unpublished RVs, and found that the comp
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Books on the topic "Stars: individual: BY Cam"

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Gründler, Gabriela. Stars of suburbia. Edition Patrick Frey, 2001.

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Bilhana. Black marigolds: And, Coloured stars. Anvil Press Poetry, 2004.

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Yosano,Akiko 与謝野,晶子 (1878-1942). River of stars: Selected poems of Yosano Akiko. Shambhala Publications, 1996.

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Panteleev, Andrey, Natal'ya Savost'yanova, and Natal'ya Fedorova. Mathematical analysis. INFRA-M Academic Publishing LLC., 2020. http://dx.doi.org/10.12737/1077332.

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The manual contains a brief statement of the course of mathematical analysis. In contrast to existing academic literature textbook starts with a Chapter on "Basic mathematics" that covers arithmetic and algebra, i.e. the essential information needed when solving problems of higher mathematics. Along with theoretical material all the sections are accompanied by a number of examples, including illustrating the geometric and economic meanings of the introduced concepts, methods and algorithms for solving mathematical, engineering and economic challenges. Given tasks for independent solving with a
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Grundler, Gabriela, and Gabriela Grindler. Stars of Suburbia. Scalo Publishers, 2001.

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A, Matilsky Terry, and United States. National Aeronautics and Space Administration., eds. Ultraviolet properties of individual hot stars in globular cluster cores. National Aeronautics and Space Administration, 1992.

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Rigby and Elsie Nelley. Rigby PM Stars: Individual Student Edition Yellow Kris's Family. Rigby Education, 2012.

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Rigby and Debbie Croft. Rigby PM Stars: Individual Student Edition Red the Race. Rigby Education, 2012.

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Smith, Annette, and Rigby. Rigby PM Stars: Individual Student Edition Red Lily's Apple. Rigby Education, 2012.

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Rigby PM Stars: Individual Student Edition Green A Firefighter. RIGBY, 2012.

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Book chapters on the topic "Stars: individual: BY Cam"

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Unsöld, Albrecht, and Bodo Baschek. "The Sun and Stars. Astrophysics of Individual Stars." In Heidelberg Science Library. Springer Berlin Heidelberg, 1991. http://dx.doi.org/10.1007/978-3-662-02681-6_4.

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Vincze, I. "Application of Deutsch’s Method for 53 Cam." In Upper Main Sequence Stars with Anomalous Abundances. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4714-6_21.

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Sills, Alison. "Models of Individual Blue Stragglers." In Ecology of Blue Straggler Stars. Springer Berlin Heidelberg, 2014. http://dx.doi.org/10.1007/978-3-662-44434-4_12.

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Zeilik, Michael, Cecila De Blasi, Michael Rhodes, and Edwin Budding. "45 years of starspot activity on SV CAM." In Cool Stars, Stellar Systems, and the Sun. Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/3-540-18653-0_185.

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Barbuy, B. "Abundances in Individual Stars of the Galactic Bulge." In Galaxy Evolution: Connecting the Distant Universe with the Local Fossil Record. Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4213-7_67.

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LoBue, Robert M. "Start-Up Investor Governance Case." In Management for Professionals. Springer International Publishing, 2021. http://dx.doi.org/10.1007/978-3-030-48606-8_3.

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AbstractIn the current age of innovative business financing opportunities available from fintech apps, social media crowdfunding sites such as Kickstarter, Indiegogo, and RocketHub, et.al., and friends and family private equity investors, start-up firms can strategically source their venture capital funds from many globally disperse organizations and individuals. As the firm in this case learned, the benefit of alternative investing sources comes with a critical hidden risk for corporate governance. After a financial restructuring, a typical Silicon Valley software start-up found itself with close to 300 external individual shareholders, some of whom had not been documented as accredited investors. The regulatory agency could decide that the prior actions of the founders and the decisions of the board had been prejudicial to the interests of the minority investors. The management of this small private company faced an atypical investor relations dilemma, before its initial public offering (IPO).
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Yi, Jiyune, R. S. Booth, and J. E. Conway. "Phase Dependence of 43 GHz SiO Masers in the Mira Variable TX Cam." In Mass-Losing Pulsating Stars and their Circumstellar Matter. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0139-7_68.

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Polosukhina, N. S., V. P. Malanushenko, I. Tuominen, H. Karttunen, and H. Virtanen. "Investigations of the Magnetic Star 53 Cam Variations using the Spectra of High Time Resolution." In Upper Main Sequence Stars with Anomalous Abundances. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4714-6_41.

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Gavryusev, V. G., and E. A. Gavryuseva. "Line Profiles and Rotational Splitting of Individual P-Modes." In New Eyes to See Inside the Sun and Stars. Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-4982-2_32.

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Luri, X., M. O. Mennessier, F. Figueras, and J. Torra. "Group identification and individual assignation of stars from kinematical and luminosity parameters." In New Approaches in Classification and Data Analysis. Springer Berlin Heidelberg, 1994. http://dx.doi.org/10.1007/978-3-642-51175-2_78.

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Conference papers on the topic "Stars: individual: BY Cam"

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Sellgren, K., D. N. B. Hall, S. G. Kleinmann, and N. Z. Scoville. "Kinematics of individual stars in the Galactic Center." In AIP Conference Proceedings Volume 155. AIP, 1987. http://dx.doi.org/10.1063/1.36404.

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Lee, Chen-Han, Lingyun Lu, Jon Dym, and Guangyan Yin. "Shape Preserving Global Parameterization for CAD/CAM/CAE." In ASME 2004 International Mechanical Engineering Congress and Exposition. ASMEDC, 2004. http://dx.doi.org/10.1115/imece2004-60274.

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CAD/CAM/CAE applications often deal with open or closed shells of faces (surfaces). Each face has it’s own 2-D parameter space that may not be rectangular. In many applications we need to merge the individual parameter spaces into a single global parameter space that resembles the model shape in the 3-D physical space. In this paper, we present a method of building such shape-preserving global parameterization (of a shell of faces) that is suitable for CAD/CAM/CAE applications.
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Van Blarigan, Benjamin, Matthew I. Campbell, Ata A. Eftekharian, and Tolga Kurtoglu. "Automated Estimation of Time and Cost for Determining Optimal Machining Plans." In ASME 2012 International Design Engineering Technical Conferences and Computers and Information in Engineering Conference. American Society of Mechanical Engineers, 2012. http://dx.doi.org/10.1115/detc2012-70338.

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In any manufacturing setting, producing a machined part is a complicated, multi-step process. It requires coordination between an engineer and a machinist to ensure all goals are met. A machinist creates a part based generally on personal experience and intuition, and while they know that this will result in the finished product, it is not guaranteed that the process plan chosen is the quickest or least expensive way to make the part. In the past year, we have been developing an automated tool that analyzes a solid model to determine its best process plan. The tool is essentially comprised of
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Cheng, Hong-Yih, and Hong-Sen Yan. "Stochastic Tolerance Synthesis for Globoidal Cam Mechanisms With the Least Manufacturing Cost." In ASME 1998 Design Engineering Technical Conferences. American Society of Mechanical Engineers, 1998. http://dx.doi.org/10.1115/detc98/mech-5822.

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Abstract This paper proposes a systematic process to analyze the mechanical error and to synthesize the tolerances for individual dimensions of spatial cam mechanisms. The mathematical expressions of geometry surface of the cam are determined by the generating method. Based on these expressions and Taylor’s series expansion, the output variables are expressed by sensitivity factors and the mean of design variables. And, the mechanical error is also calculated according to the measured coordinate data on the manufactured cam surface and misalignments. By applying statistics and cost-tolerance f
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Yu, Ying-Ju, and Chin-Hsiang Cheng. "Dynamic Simulation of a Beta-Type Stirling Engine With Cam-Drive Mechanism." In ASME 2010 International Mechanical Engineering Congress and Exposition. ASMEDC, 2010. http://dx.doi.org/10.1115/imece2010-40635.

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Dynamic simulation of a beta-type Stirling engine with cam-drive mechanism has been performed. A dynamic model associated with the cam-drive mechanism has been developed. Upon obtaining the gas pressure inside the chambers, the derived dynamic model is used to evaluate the transient rotational speed of the engine before the steady-state regime is reached. The torque of the engine can be calculated as long as the gas force, the inertia torque, the friction torque, and the load torque are evaluated. In this study, the mass moment of inertia of the flywheel is firstly calculated. The friction tor
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Zhao, Zhengcai, Yucan Fu, Jiuhua Xu, and Yong Chen. "Measurement-Based Adaptive Machining by Direct Spatial Deformation of Template CAM Data." In ASME 2017 12th International Manufacturing Science and Engineering Conference collocated with the JSME/ASME 2017 6th International Conference on Materials and Processing. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/msec2017-2773.

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In production and manufacturing engineering, some redesign, distorted or worn parts cannot be milled according to their original CAD geometries due to the existed shape deviations. Generating CAM data in traditional manner for each individual part is time-consuming and labor intensive. This paper proposes a quick and convenient adaptive approach for machining distorted hollow blade, in which a template CAM data is spatially deformed according to some measured points from actual shape. The actual shape of the part was firstly inspected by on-machine measurement method. The measured points data
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Datta, Debashis, and Changheui Jang. "Incorporation of Materials’ Sensitive Simulation Technique Into the PINTIN-CAM Code for Integrity of Nuclear Piping System." In ASME 2010 Pressure Vessels and Piping Division/K-PVP Conference. ASMEDC, 2010. http://dx.doi.org/10.1115/pvp2010-25395.

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Previously, the development process of a combined probabilistic fracture mechanics code for nuclear piping system was proposed based on some pre-assigned (by default) crack initiation and crack growth techniques e.g. assumption of preexisting cracks in case of no initiated cracks resulted from either fatigue or stress corrosion crack mechanisms and individual growth of those cracks by fatigue or stress corrosion cracking phenomenon without considering crack coalescence criteria. In one sense this type of approach might produce conservative results. To reduce the undue conservatism, in this ver
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Lenzi, Tommaso, Marco Cempini, Levi Hargrove, and Todd Kuiken. "Hybrid Actuation Systems for Lightweight Transfemoral Prostheses." In 2017 Design of Medical Devices Conference. American Society of Mechanical Engineers, 2017. http://dx.doi.org/10.1115/dmd2017-3398.

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Lower-limb amputation affects the ambulation ability and quality of life of about 600,000 individuals in the United States alone1. Individuals with transfemoral amputation typically walk slower, expend more energy, and have a higher risk of falls than able-bodied individuals2. Ambulation activities such as climbing ramps or stairs or standing up from a seated position are much more difficult than for able-bodied persons. Advances in prosthetic technologies are needed to improve the ambulation ability of above-knee amputees. Passive knee prostheses are lightweight, robust, and quiet, but can on
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Hamade, R. F. "Studying Your Students as They Learn: A Case Study of CAD Education." In ASME 2009 International Mechanical Engineering Congress and Exposition. ASMEDC, 2009. http://dx.doi.org/10.1115/imece2009-10195.

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Having observed mechanical engineering seniors at the American University of Beirut (AUB) go about learning computer-aided design (CAD) in a formal setting, the instructors always wondered why some students acquire CAD skills with relative ease while some others seem to struggle. For this reason, a methodical study was launched in order to address this issue. Hence, and in order to “study the students as they learn” was accomplished by following 74 mechanical engineering seniors (it took three academic years including AY 2008–09 in order to have access to this relatively large number of traine
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Orčić, Drago. "How to Detect Hidden Individual Potential (intellectual DNA) of an Entrepreneur." In Organizations at Innovation and Digital Transformation Roundabout. University of Maribor Press, 2020. http://dx.doi.org/10.18690/978-961-286-388-3.41.

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Entrepreneurship is a powerful tool in the value creation function. Contemporary trends indicate that entrepreneurship is not so much a matter of choice but it is increasingly an issue of survival. In the age of knowledge, intellectual potential becomes a key segment of successful entrepreneurship. The discovery, development and management of intellectual potential gives entrepreneurs, in addition to a competitive edge in the modern market, a greater chance of success in developing an entrepreneurial idea. According to research, in the first three years of business, about 90% of start-ups fail
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Reports on the topic "Stars: individual: BY Cam"

1

McKenna, Patrick, and Mark Evans. Emergency Relief and complex service delivery: Towards better outcomes. Queensland University of Technology, 2021. http://dx.doi.org/10.5204/rep.eprints.211133.

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Emergency Relief (ER) is a Department of Social Services (DSS) funded program, delivered by 197 community organisations (ER Providers) across Australia, to assist people facing a financial crisis with financial/material aid and referrals to other support programs. ER has been playing this important role in Australian communities since 1979. Without ER, more people living in Australia who experience a financial crisis might face further harm such as crippling debt or homelessness. The Emergency Relief National Coordination Group (NCG) was established in April 2020 at the start of the COVID-19 p
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2

Shaping the COVID decade: addressing the long-term societal impacts of COVID-19. The British Academy, 2021. http://dx.doi.org/10.5871/bac19stf/9780856726590.001.

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In September 2020, the British Academy was asked by the Government Office for Science to produce an independent review to address the question: What are the long-term societal impacts of COVID-19? This short but substantial question led us to a rapid integration of evidence and an extensive consultation process. As history has shown us, the effects of a pandemic are as much social, cultural and economic as they are about medicine and health. Our aim has been to deliver an integrated view across these areas to start understanding the long-term impacts and how we address them. Our evidence revie
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