Relevant bibliographies by topics / Astrophysics and Space Science

Contents

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

Academic literature on the topic 'Astrophysics and Space Science'

Author: Grafiati
Published: 4 June 2021
Last updated: 8 February 2022

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Journal articles on the topic "Astrophysics and Space Science"

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Dopita, Michael A. "Astrophysics & Space Science editorial." Astrophysics and Space Science 312, no. 1-2 (October 5, 2007): 1–2. http://dx.doi.org/10.1007/s10509-007-9652-z.

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Zheleznyakov, V. V. "New Books: Astrophysics and Space Science." Physics Essays 10, no. 3 (September 1997): 534–35. http://dx.doi.org/10.4006/1.3041626.

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Makishima, Kazuo. "Space Astrophysics in Japan." Publications of the Astronomical Society of Australia 9, no. 1 (1991): 57–59. http://dx.doi.org/10.1017/s1323358000024887.

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Riegler, Guenter R. "Science Operations for Future Space Astrophysics Missions." International Astronomical Union Colloquium 123 (1990): 317–21. http://dx.doi.org/10.1017/s0252921100077228.

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AbstractPlans for astrophysics science operations during the decade of the nineties are described from the point of view of a scientist who wishes to make a space-borne astronomical observation or to use archival astronomical data. In the process of preparing a proposal, making an observation, and carrying out data processing, analysis, and dissemination of results, the scientist will be able to use a variety of services and infrastructure, including the “Astrophysics Data System”. The current status and plans for these science operations services are described.
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Stankus, Tony. "Astronomy, Astrophysics, and Space Sciences." Serials Librarian 27, no. 2-3 (April 8, 1996): 59–65. http://dx.doi.org/10.1300/j123v27n02_04.

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Glanz, J. "ASTROPHYSICS: X-rays Hint at Space Pirouette." Science 278, no. 5340 (November 7, 1997): 1012b—1013. http://dx.doi.org/10.1126/science.278.5340.1012b.

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Irion, R. "ASTROPHYSICS: Stanford Gets Serious About Space Physics." Science 299, no. 5606 (January 24, 2003): 492b—492. http://dx.doi.org/10.1126/science.299.5606.492b.

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Agnello, S. Dell’, G. Delle Monache, R. Vittori, A. Boni, C. Cantone, E. Ciocci, M. Martini, et al. "Advanced Laser Retroreflectors for Astrophysics and Space Science." Journal of Applied Mathematics and Physics 03, no. 02 (2015): 218–27. http://dx.doi.org/10.4236/jamp.2015.32032.

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Lawler, A. "Astronomy and Astrophysics: Crunch Ahead for Space Science." Science 271, no. 5256 (March 22, 1996): 1660b—1661. http://dx.doi.org/10.1126/science.271.5256.1660b.

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Kestenbaum, D. "ASTROPHYSICS: X-ray Flickers Reveal a Space Warp." Science 280, no. 5364 (May 1, 1998): 674–75. http://dx.doi.org/10.1126/science.280.5364.674.

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Dissertations / Theses on the topic "Astrophysics and Space Science"

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Bonokwane, Kelebogile. "SALT and TESS monitoring of central stars of planetary nebulae." Master's thesis, Faculty of Science, 2021. http://hdl.handle.net/11427/33436.

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Planetary Nebulae (PNe) are the product of Asymptotic Giant Branch (AGB) evolution. Evolved from Solar-like intermediate mass stars (0.8 – 8M), they have a hot, radiating core that ionizes the gas of the expelled envelope, producing a glowing nebula. The core eventually evolves into a white dwarf (WD), following the WD cooling track. Complex, aspherical morphologies are observed in PNe and binary central stars (CSs) have been the favoured explanation for deviations from spherical symmetry. Finding and characterizing the population of binary CSs is thus important to understand the physics behind their morphologies. The objects of this study are Hen3-1333, Hen2-113 and Hen2-47, all with WolfRayet (WR) CSs that commonly exhibit fast, dense stellar winds. All exhibit multipolarity in their young nebulae, Hen3-1333 has a disk and dual-dust chemistry, while the other two have central stars offset from the geometric centre of their nebulae. The objects were chosen because most of these features, especially multipolar morphologies, are not well represented amongst PNe with known binary CSs. Here we develop a quantitative time-series analysis to determine whether these objects have binary CSs and develop constraints to permissible orbital parameters. The High Resolution Spectrograph (HRS) of the Southern African Large Telescope (SALT) was used to collect échelle spectroscopic data over 3 years and The Exoplanet Survey Satellite (TESS) was used to obtain photometric data for the objects. The medium resolution (MR) mode (R ≈ 40000) was chosen and 58, 60, and 35 spectra were collected for Hen3-1333, Hen2-113 and Hen2-47, respectively, with an average S/N of 40 at 4495 Å. The TESS data had continuous sampling (30 min cadence) recorded for an orbit length of 27.4 days. Using cross-correlation and Gaussian line fitting, radial velocity (RV) time-series were compared to lightcurves determined from the TESS data. Lomb-Scargle periodograms were used to search for periodic variability in the RV and photometry time-series data. The results were discussed based on short (0 – 10 days), intermediate (10 – 103 days) and long (103 – 104 days) orbital period ranges. Compatible scenarios for each range were estimated by combining observational constraints with different parameters expected for assumed companion star types. The quantitative variability analysis excludes short orbital period binary systems, suggesting that if their multiple features are due to binary interactions, the most likely case is the long orbital period range. If the variability observed is due to a companion, rather than pulsations from the CS, the companion masses, 0.10 – 1.36 M for Hen3-1333, 0.043 – 1.27 M for Hen2-113 and 0.077 – 1.36 M for Hen2-47, correspond to main sequence stars and dwarfs.
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Oreta, Timothy. "Vector-Galileon-Tensor theories of gravity." Master's thesis, University of Cape Town, 2016. http://hdl.handle.net/11427/20925.

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A detailed study of the cosmological evolution in a particular vector-tensor theory of gravity with a potential and a Galileon-motivated interaction terms is presented. The evolution of vector field self interactions that are relatively related to Galileon fields throughout the expansion history of the universe is considered and a classification of the parameters M (mass term) and H (Hubble parameter) according to the behaviour of the field in each cosmological epoch is carried out. In particular, we obtain conditions for the parameters so that the field grows exponentially or oscillates with decreasing amplitude. We also obtain an autonomous system for the inflationary case. The general features of the phasemaps are given and the critical point is appropriately characterised. It is not possible to obtain an autonomous system for radiation and matter dominated epochs hence, we consider other analytical methods. We obtain eigenvalues and hence, phasemaps. The general features of the phasemaps are given and the point to which the trajectories on the phasemaps converge is appropriately characterised. Therefore, we show that it is possible to obtain a wide variety of behaviours or interesting phenomenologies for the cosmological evolution of vector field self-interactions that are relatively related to Galileon fields by choosing suitable values for the parameters M and H of given conditions.
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Misra, Anuj. "Towards a holographic description of pulsar glitch mechanism." Master's thesis, University of Cape Town, 2015. http://hdl.handle.net/11427/15589.

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This work aims to review the progress in understanding the underlining physics of pulsar glitches: beginning from the pedagogical development of the subject to eventually motivating the use of AdS/CFT techniques in studying a certain class of condensed matter systems. The foundation of this work is built upon the Gross Pitaevskii (GP) model of super-fluidity applied to the interior matter of neutron stars, where the condensate wave function acts as the order parameter of the macroscopic coherence theory. The excitation modes of the field equations are found to be solitonic vortices, which then go on to present a theoretical basis to the plausible theories of pulsar glitches involving vortex dynamics. The second major thrust of this thesis is in reviewing the application of AdS/CFT in study of strongly-coupled condensed matter systems, with special attention to the models of holographic superfluidity that admit vortex-like solutions. The basic identification of the characteristic free energy configuration of global vortices in the AdS/CFT prescription enables to motivate its use in studying the pulsar glitch mechanism. The last part of this work traces the conclusions of this review and attempts to present the current state-of-progress of the field with its extensive domain of purview and open lines of inquiry.
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Kubwimana, Jean Claude. "Cosmic acceleration and the coincidence problem." Master's thesis, University of Cape Town, 2009. http://hdl.handle.net/11427/6102.

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In the standard model of the Universe, the cosmos has only accelerated once since decoupling and only recently, at around a redshift of z ̃ 0.5 as supported by different observations including Type Ia Supernovae (SNIa), the Cosmic Microwave Background (CMB), Large Scale Structure (LSS), and Weak Lensing (WL). This confirmation however, lacks a fundamental physics explanation. The hypothetical form of energy termed 'dark energy' (DE) assumed to account for that acceleration behavior, is still mysterious and why its dominance only occurred recently is a profound problem widely known as the coincidence problem. So far all attempts for resolving the coincidence the problem have been unsatisfactory. Here we investigate a possible solution to the coincidence problem in the form of multiples phases of acceleration (MPA). If there were more than one phase of acceleration between now and decoupling, then the current phase of acceleration would be much less special, alleviating the coincidence problem. We use a modified Markov Chain Monte Carlo (MCMC) technique together with the WMAP five year TT data to search for parameters allowing a second phase of acceleration. Despite extensive search we find no models that simultaneously fit the WMAP data and yield a second phase of acceleration, ruling out this particular set of models as the solution to the coincidence problem.
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Obonyo, Willice Odhiambo. "Open clusters and HII regions of our Galaxy." Master's thesis, University of Cape Town, 2015. http://hdl.handle.net/11427/19997.

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Open clusters are essential laboratories for understanding stellar evolution, as they allow constraints to be placed on stellar ages and luminosities. As distance indicators they are also important tracers of star formation in the Milky Way. One such cluster is Trumpler 27 that we identified for detailed study.The aim of the study is to estimate the distance, radial velocity, age, membership and reddening of the cluster using both spectroscopic and photometric techniques. We used new spectroscopic data collected from SAAO's 1.9m telescope together with existing photometric data from catalogues in the study of Trumpler 27. The spectra collected were classified using spectral atlases to determine the reddening in the field. Stars of the cluster were identified using selection techniques that made use of both infrared and optical Q parameters, spatial distribution and photometric techniques. The result from this work suggest that Trumpler 27 is made up of ~ 55 stars which are at different stages of evolution. The stars include main sequence stars, blue supergiants, two cool supergiants and maybe two WR stars.
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Tapsoba, Wendyam Blaise. "Analysis of SALT Fabry-Pérot medium resolution data." Master's thesis, University of Cape Town, 2015. http://hdl.handle.net/11427/16494.

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The Southern African Large Telescope Fabry-Pérot interferometer has been used in its medium resolution mode to observe three of 30 galaxies of the MHONGOOSE galaxy sample for which very deep HI observation (typically 200 hours/galaxy) will be obtained with MeerKAT. So optical high spatial resolution of 2 arcsec data of NGC 7361, NGC 7424 and NGC 7793 have been obtained. The major object of this thesis was to test SALT Fabry-Pérot medium resolution data in order to pursue the survey of all the MHONGOOSE sample, and to be able to compare the accuracy of the kinematic results. Through this work, some FORTRAN based routines have been improved and they allow us to compute kinematic maps with good accuracy. Indeed, the velocities measured from the profiles of the Hα emission in the data cube are accurate with the range of 1 km s⁻¹ to 10 km s⁻¹. So, we computed the kinematic maps and the rotation curves of the three galaxies using DiskFit and ROTCUR. For NGC 7361 and NGC 7424 we compared the rotation curves derived by both methods. For NGC 7793 we were also able to compare our results with previous studies.
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Tshenye, Thapelo Obed. "Quality control of astronomical CCD observations." Master's thesis, University of Cape Town, 2007. http://hdl.handle.net/11427/4409.

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Okouma, Patrice M. "Type Ia supernovae as tools for cosmology." Master's thesis, University of Cape Town, 2008. http://hdl.handle.net/11427/4424.

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Sikhonde, Muzikayise E. "A study of chameleon-photon mixing from pulsars." Master's thesis, University of Cape Town, 2012. http://hdl.handle.net/11427/12638.

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A number of solutions to the dark energy problem have been proposed in literature, the simplest is the cosmological constant A. The cosmological constant lacks theoretical explanation for its extremely small value, thus dark energy is more generally modelled as a quintessence scalar field rolling down a flat potential.
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Affadi, Ikechukwu Patrick. "A new method of mapping cosmic flow fields : evaluating the sustainability of the infrared bands Tully-Fisher relation for ZoA work." Master's thesis, University of Cape Town, 2016. http://hdl.handle.net/11427/20813.

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This thesis aims at using the Infrared Survey Facility (IRSF) JHKₛ bands, Two Micron All Sky Survey (2MASS) JHKₛ bands and Wide Field Infrared Survey Explorer (WISE) W1-W4 bands isophotal magnitudes to understand the cosmic flow associated with Zone of Avoidance (ZoA) galaxies.
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Books on the topic "Astrophysics and Space Science"

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Maccarone, T. J., R. P. Fender, and L. C. Ho, eds. Astrophysics and Space Science. Dordrecht: Springer Netherlands, 2005. http://dx.doi.org/10.1007/1-4020-4085-7.

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Dyson, John, Susan A. Lamb, A. G. W. Cameron, A. M. Cherepashchuk, C. G. Fälthammar, M. Kitamura, L. B. F. M. Waters, C. Waelkens, K. A. van der Hucht, and P. A. Zaal, eds. Astrophysics and Space Science. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5076-7.

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Astrophysical jets and beams. Cambridge: Cambridge University Press, 2012.

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1972-, Brüggen Marcus, ed. Introduction to high-energy astrophysics. New York, NY: Cambridge University Press, 2007.

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Canary Islands) Canary Islands Winter School on Astrophysics (21st 2009 Puerto de la Cruz. Accretion processes in astrophysics: XXI Canary Islands Winter School of Astrophysics. New York, NY, USA: Cambridge University Press, 2014.

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Smith, Michael D. Astrophysical jets and beams. Cambridge: Cambridge University Press, 2012.

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Space. Mankato, Minn: Sea-to-Sea Publications, 2011.

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Morrison, D. Space Science Division cumulative bibliography, 1989-1994. Moffett Field, Calif: National Aeronautics and Space Administration, Ames Research Center, 1995.

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Morrison, D. Space Science Division cumulative bibliography, 1989-1994. Moffett Field, Calif: National Aeronautics and Space Administration, Ames Research Center, 1995.

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author, Kregenow Julia, ed. Astrophysics for babies. Naperville, Illinois]: Sourcebooks, Incorporated, 2018.

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Book chapters on the topic "Astrophysics and Space Science"

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Somov, Boris V. "Magnetohydrodynamics in Astrophysics." In Astrophysics and Space Science Library, 263–83. New York, NY: Springer New York, 2012. http://dx.doi.org/10.1007/978-1-4614-4283-7_13.

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Read, M., B. Mann, R. Blake, R. Collins, N. Cross, C. Davenhall, M. Holliman, and E. Sutorius. "Science Archives: Facilitating Survey Science." In Astrophysics and Space Science Proceedings, 61–65. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-19330-4_8.

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Chattopadhyay, Indranil. "Relativistic Flows in Astrophysics." In Astrophysics and Space Science Proceedings, 17–27. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-94607-8_2.

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Perrin, Guy. "VLTI Science Highlights." In Astrophysics and Space Science Proceedings, 81–87. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9190-2_14.

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Sinha, K. "My “Science Mother”." In Astrophysics and Space Science Library, 126–27. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5173-3_42.

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Krishan, Vinod. "Astrophysical Quantities." In Astrophysics and Space Science Library, 339–42. Dordrecht: Springer Netherlands, 1999. http://dx.doi.org/10.1007/978-94-011-4720-0_9.

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Santos, Nuno C., and João P. Faria. "Exoplanetary Science: An Overview." In Astrophysics and Space Science Proceedings, 165–80. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-59315-9_9.

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Martens, Petrus C. "Soho — Yohkoh Science Collaboration." In Astrophysics and Space Science Library, 217–26. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5220-4_36.

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Sarkar, Shyam, Ashim Sarkar, and Pabitra Sil. "Science with Small Telescopes." In Astrophysics and Space Science Proceedings, 387–94. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-94607-8_30.

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Benz, Arnold. "Astrophysical Electron Beams." In Astrophysics and Space Science Library, 115–53. Dordrecht: Springer Netherlands, 1993. http://dx.doi.org/10.1007/978-94-011-2064-7_6.

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Conference papers on the topic "Astrophysics and Space Science"

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Rudnitskiy, Alexey, Sergey Likhachev, Andrey Andrianov, Vladimir I. Kostenko, and Yuri Schekinov. "The Current and Future of Ground and Space-VLBI Science." In Frontier Research in Astrophysics – III. Trieste, Italy: Sissa Medialab, 2019. http://dx.doi.org/10.22323/1.331.0084.

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Nikzad, Shouleh. "Enabling technologies for astrophysics, planetary science, and terrestrial applications." In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XXII, edited by Oswald H. Siegmund. SPIE, 2021. http://dx.doi.org/10.1117/12.2603698.

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Good, J. C., and R. B. Pomphrey. "Overview of the astrophysics data system (ADS)." In The earth and space science information system (ESSIS). AIP, 1993. http://dx.doi.org/10.1063/1.44410.

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Michelson, Peter F. "The Gamma-ray large area space telescope mission: Science opportunities." In GAMMA 2001: Gamma-Ray Astrophysics 2001. AIP, 2001. http://dx.doi.org/10.1063/1.1419488.

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Elvis, Martin. "The Crisis in Space Astrophysics and Planetary Science: How Commercial Space and Program Design Principles will let us Escape." In Frontier Research in Astrophysics – II. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.269.0066.

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Siegmund, Oswald H. W., Anton S. Tremsin, and John V. Vallerga. "High performance cross-strip detector technologies for space astrophysics." In 2007 IEEE Nuclear Science Symposium Conference Record. IEEE, 2007. http://dx.doi.org/10.1109/nssmic.2007.4436595.

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Jones, Dayton, and Joseph Lazio. "Enhancing Science from Future Space Missions and Planetary Radar with the SKA." In Advancing Astrophysics with the Square Kilometre Array. Trieste, Italy: Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.215.0154.

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Djorgovski, S. G., A. A. Mahabal, D. J. Crichton, and B. Chaudhry. "From stars to patients: Lessons from space science and astrophysics for health care informatics." In 2015 IEEE International Conference on Big Data (Big Data). IEEE, 2015. http://dx.doi.org/10.1109/bigdata.2015.7364135.

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Cherry, Michael L., Peter P. Altice, Jr., Steven B. Ellison, T. Gregory Guzik, John R. Macri, Mark L. McConnell, G. Y. McLean, James M. Ryan, and Paul P. Suni. "Charge-coupled devices with fast timing for astrophysics and space physics research." In SPIE's 1996 International Symposium on Optical Science, Engineering, and Instrumentation, edited by Brian D. Ramsey and Thomas A. Parnell. SPIE, 1996. http://dx.doi.org/10.1117/12.254006.

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Grygar, J. "The role of space-based observations in astrophysical research." In Basic space science. AIP, 1992. http://dx.doi.org/10.1063/1.41711.

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Reports on the topic "Astrophysics and Space Science"

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W Matthaeus and M Brown. Turbulent Magnetohydrodynamic Acceleration Processes: Theory SSX Experiments and Connections to Space and Astrophysics. Office of Scientific and Technical Information (OSTI), July 2006. http://dx.doi.org/10.2172/886953.

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Fenimore, Edward E. 50 years of science from space. Office of Scientific and Technical Information (OSTI), February 2015. http://dx.doi.org/10.2172/1095225.

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Koedinger, Kenneth R., Daniel D. Suthers, and Kenneth D. Forbus. Component-Based Construction of a Science Learning Space. Fort Belvoir, VA: Defense Technical Information Center, January 1998. http://dx.doi.org/10.21236/ada638366.

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Kowalski, Michael P., Martin Barstow, Frederick Bruhweiler, Raymond Cruddace, Andrea Dupree, Jay Holberg, Steve Howell, et al. Million Degree Plasmas in Extreme Ultraviolet (EUV) Astrophysics. White Paper in Response to Astro2010 Science Call. Fort Belvoir, VA: Defense Technical Information Center, January 2010. http://dx.doi.org/10.21236/ada520713.

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Perry, Scott S. Miniaturization Science for Space: Lubrication of Micro-Electro-Mechanical Systems (MEMS) for Space Environments. Fort Belvoir, VA: Defense Technical Information Center, August 2006. http://dx.doi.org/10.21236/ada458531.

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Yen, Chen-wan L. Nuclear electric propulsion for future NASA space science missions. Office of Scientific and Technical Information (OSTI), July 1993. http://dx.doi.org/10.2172/10102393.

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Church, Michael Kenton, and Benn Tannenbaum. Testimony to the House Science Space and Technology Committee. Office of Scientific and Technical Information (OSTI), March 2018. http://dx.doi.org/10.2172/1426550.

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Nelson, Jenenne. (Congressional Interest) Institute for Science, Space and Security (ISSS). Fort Belvoir, VA: Defense Technical Information Center, March 2012. http://dx.doi.org/10.21236/ada579363.

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Dahlburg, Jill P., George A. Doschek, James D. Kurfess, Judith L. Lean, David E. Siskind, and Dennis G. Socker. Naval Research Laboratory Space Science Division Newsletter: 01/2007. Fort Belvoir, VA: Defense Technical Information Center, April 2007. http://dx.doi.org/10.21236/ada467316.

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Wagner, P. Material science experience gained from the space nuclear rocket program: Insulators. Office of Scientific and Technical Information (OSTI), July 1992. http://dx.doi.org/10.2172/6736381.

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