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Gotowe bibliografie tematyczne / Observational astronomy

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Gotowa bibliografia na temat „Observational astronomy”

Autor: Grafiati

Data publikacji: 4 czerwca 2021

Data aktualizacji: 27 kwietnia 2022

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Artykuły w czasopismach na temat "Observational astronomy"

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Kim, Yong H. "Teaching Observational Astronomy as a Laboratory Course for Non-Majors." International Astronomical Union Colloquium 105 (1990): 154–58. http://dx.doi.org/10.1017/s0252921100086620.

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Since antiquity, doing astronomy means basically stepping outside, looking upward, and considering the widest environment. Thus any undergraduate astronomy program, no matter how diverse its course offering, is incomplete without observational astronomy. For example, some California community colleges offer several courses including such titles as “Man and the Cosmos,” “Final Stellar States,” “Astronomy Enrichment,” and “Astronomical Myths, Mysteries & Fallacies,” but do not offer “Observational Astronomy.” As a teaching astronomer, I question the wisdom and honesty of such practice of pro

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Surdin, V. G. "Observational Astronomy: Status 2020." Physics of Atomic Nuclei 83, no. 6 (November 2020): 962–64. http://dx.doi.org/10.1134/s1063778820050191.

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TAMURA, Motohide. "New Frontiers of Observational Astronomy." Journal of the Visualization Society of Japan 15, no. 59 (1995): 240–45. http://dx.doi.org/10.3154/jvs.15.59_240.

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Arp, Halton. "Observational Problems in Extragalactic Astronomy." Highlights of Astronomy 9 (1992): 43–62. http://dx.doi.org/10.1017/s153929960000873x.

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AbstractA large number of observations have accumulated which represent baffling mysteries from the standpoint of current astronomy. A sample of the most crucial of these cases is reviewed and updated. Evidence has slowly built up to the point where often each individual object is a formidable challenge to conventional theory. But, most importantly, it is now possible to appreciate the common pattern which mutually reinforces all the separate results.These empirical discordances point directly at known weaknesses in the Big Bane theory of the origin of the universe. New data is used to introdu

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Batten, Alan H. "Observational Astronomy in New Zealand." Journal for the History of Astronomy 46, no. 4 (October 30, 2015): 496–97. http://dx.doi.org/10.1177/0021828615593271.

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Zdor, Ye S., and V. S. Chernov. "Space ecology and observational astronomy." Astronomical & Astrophysical Transactions 4, no. 1 (June 1993): 47–48. http://dx.doi.org/10.1080/10556799308205361.

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CANIZARES, C. R. "High-Tech Astronomy: Observational Astrophysics." Science 244, no. 4906 (May 19, 1989): 851. http://dx.doi.org/10.1126/science.244.4906.851.

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Bravo-Alfaro, Hector. "An Undergraduate Program for Astronomy in México." Transactions of the International Astronomical Union 24, no. 3 (2001): 164–65. http://dx.doi.org/10.1017/s0251107x00000614.

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Astronomy in México has an ancient tradition, reinforced during the twentieth century by groups working in theoretical and observational astronomy. During the 1990s, the Great Millimeter Telescope (a single 50-m antenna) has been approved, and a 6-m infrared telescope is under study. Graduate and undergraduate programs must be improved to prepare future Mexican and Latin American astronomers to take advantage of these facilities. To meet the challenge, two traditional Mexican programs (Instituto de Astronomia-UNAM and Instituto Nacional de Astrofisica, Optica y Electronica-INAOE) are updating

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Govind, Amith, Devarshi Choudhury, Blesson Mathew, and Paul K. T. "Astrometry: The Foundation for Observational Astronomy." Mapana - Journal of Sciences 17, no. 1 (January 1, 2018): 1–10. http://dx.doi.org/10.12723/mjs.44.1.

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Astronomy has seen unprecedented growth in the past century, due to the rise in multiwavelength observations. The foundation for multiwavelength astronomy is given by Astrometry; the science of position and motion determination of celestial bodies. We present a technique of determining equatorial coordinates of celestial bodies from their pixel coordinates. We also present the subsequent results of using this technique in achieving the initial few steps required for the multiwavelength studies of young open clusters.

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Maffie, James. "Watching the Heavens with a ‘Rooted Heart’: The Mystical Basis of Aztec Astronomy." Culture and Cosmos 12, no. 1 (June 2008): 31–64. http://dx.doi.org/10.46472/cc.0112.0205.

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Aztec epistemology maintained that humans acquire knowledge of reality mystically using their hearts, not their five senses. What, then, was the epistemological status of observational astronomy? Aztec epistemology assigned a privileged role to mystical knowledge and an ancillary, propaedeutical role to observational astronomy. The epistemological evaluation of observational claims in Aztec astronomy occurred within a context of mystically rooted metaphysical, religious, and astrological background assumptions. These played an essential role in the epistemology of Aztec astronomy.

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Rozprawy doktorskie na temat "Observational astronomy"

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Widicus, Weaver Susanna Leigh Beauchamp Jesse L. "Rotational spectroscopy and observational astronomy of prebiotic molecules /." Diss., Pasadena, Calif. : California Institute of Technology, 2005. http://resolver.caltech.edu/CaltechETD:etd-05162005-153745.

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Corrigan, Ruth T. "Observational manifestations of gravitational lenses." Thesis, University of Cambridge, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.260611.

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Añez, López José Ignacio. "Observational and theoretical perspective of massive star formation." Doctoral thesis, Universitat de Barcelona, 2021. http://hdl.handle.net/10803/671784.

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In this thesis, we are aimed to better understand the massive star formation process paying special attention to the role of the magnetic field. To do this, we will carry out a multi-scale analysis with a double approach, theoretical and observational. a) The role of the magnetic field in the fragmentation process: the case of G14.225-0.506 In this first work, we study the fragmentation of an infrared dark cloud that has a filamentary structure and two hubs. We will pay special attention to the magnetic field present in the environment of the hubs and we will try to relate it to the di

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Kelly, Brandon Charles. "Observational Constraints on the Structure and Evolution of Quasars." Diss., The University of Arizona, 2008. http://hdl.handle.net/10150/193633.

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I use X-ray and optical data to investigate the structure of quasars, and its dependence on luminosity, redshift, black hole mass, and Eddington ratio. In order to facilitate my work, I develop new statistical methods of accounting for measurement error, non-detections, and survey selection functions. The main results of this thesis follow. (1) The statistical uncertainty in the broad line mass estimates can lead to significant artificial broadening of the observed distribution of black hole mass. (2) The z = 0.2 broad line quasar black hole mass function falls off approximately as a power law

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Uthas, Helena. "Observational studies of highly evolved cataclysmic variables." Thesis, University of Southampton, 2011. https://eprints.soton.ac.uk/202889/.

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Cataclysmic Variables (CV) are binary systems where a main-sequence star transfers mass onto a white dwarf (WD). According to standard evolutionary theory, angular momentum loss drives CVs to initially evolve from longer to shorter orbital periods until a minimum period is reached (≈ 80 minutes). At roughly this stage, the donors becomes degenerate, expand in size, and the systems move towards longer orbital periods. Theory predicts that 70% of all CVs should have passed their minimum period and have sub-stellar donors, but until recently, no such systems were known. I present one CV showing e

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Seigar, Marcus S. "Observational studies of the structure of spiral galaxies." Thesis, Liverpool John Moores University, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.242314.

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Nelson, Andrew Frederick. "Dynamics and observational appearance of circumstellar disks." Diss., The University of Arizona, 1999. http://hdl.handle.net/10150/288969.

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In my thesis I present a study of the dynamics and observational characteristics of massive circumstellar disks in two dimensions (r, φ) using two complimentary hydro-dynamic codes: a 'Smoothed Particle Hydrodynamic' (SPH) code and a 'Piecewise Parabolic Method' (PPM) code. I also study the detection limits available to radial velocity searches for low mass companions to main sequence stars. This thesis is organized as a series of published or submitted papers, connected by introductory and concluding material. I strongly recommend that readers of this abstract obtain the published versions of

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Stempels, Henricus Cornelis. "An Observational Study of Accretion Processes in T Tauri Stars." Doctoral thesis, Uppsala : Acta Universitatis Upsaliensis : Univ.-bibl. [distributör], 2003. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-3420.

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Endicott, Thomas G. "Effect of Observational Cadence on Orbit Determination for Synthetic Near-Earth Objects." Thesis, University of Massachusetts Boston, 2017. http://pqdtopen.proquest.com/#viewpdf?dispub=10617372.

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<p> Near-Earth Objects (NEOs) are generally small, dark, and fast-moving. Multiple observations over time are necessary to constrain NEO orbits. Orbits based on observational data are inherently uncertain. Here we describe code written in Python and Fortran used to generate synthetic asteroids and compare calculated orbital fit based on noisy ephemeris using the a distance criteria, D-value. Observational sessions separated by more than one month produce very good orbital fits (low D-values) even at the highest noise level. Daily observational sessions show the highest D-values, as expected, s

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Moffat, Anthony F. J. "Observational overview of clumping in hot stellar winds." Universität Potsdam, 2007. http://opus.kobv.de/ubp/volltexte/2008/1763/.

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In the old days (pre ∼1990) hot stellar winds were assumed to be smooth, which made life fairly easy and bothered no one. Then after suspicious behaviour had been revealed, e.g. stochastic temporal variability in broadband polarimetry of single hot stars, it took the emerging CCD technology developed in the preceding decades (∼1970-80’s) to reveal that these winds were far from smooth. It was mainly high-S/N, time-dependent spectroscopy of strong optical recombination emission lines in WR, and also a few OB and other stars with strong hot winds, that indicated all hot stellar winds likely to b

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Książki na temat "Observational astronomy"

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Birney, D. Scott. Observational astronomy. Cambridge: Cambridge University Press, 1991.

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Birney, D. Scott. Observational astronomy. Cambridge [England]: Cambridge University Press, 1991.

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Sarma, K. V. Observational astronomy in India. Kerala: Dept. of Sanskrit, University of Calicut, 1990.

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Observational astronomy: Techniques and instrumentation. Cambridge: Cambridge University Press, 2011.

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Observational astrophysics. 3rd ed. Heidelberg: Springer, 2012.

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Léna, Pierre. Observational astrophysics. 2nd ed. Berlin: Springer, 1998.

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Observational astrophysics. Berlin: Springer-Verlag, 1988.

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Dark energy: Observational and theoretical approaches. Cambridge, UK: Cambridge University Press, 2010.

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Chromey, Frederick R. To measure the sky: An introduction to observational astronomy. Cambridge: Cambridge University Press, 2010.

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To measure the sky: An introduction to observational astronomy. Cambridge: Cambridge University Press, 2010.

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Części książek na temat "Observational astronomy"

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Longair, Malcolm S. "Radio Astronomy and Cosmology." In Observational Cosmology, 3–10. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-011-5238-9_1.

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Rohlfs, K., and T. L. Wilson. "Observational Methods." In Astronomy and Astrophysics Library, 166–91. Berlin, Heidelberg: Springer Berlin Heidelberg, 1996. http://dx.doi.org/10.1007/978-3-662-03266-4_7.

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Wilson, Thomas L., and Susanne Hüttemeister. "Observational Methods." In Astronomy and Astrophysics Library, 39–44. Berlin, Heidelberg: Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-57001-8_8.

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Branch, David, and J. Craig Wheeler. "Observational Properties." In Astronomy and Astrophysics Library, 483–517. Berlin, Heidelberg: Springer Berlin Heidelberg, 2017. http://dx.doi.org/10.1007/978-3-662-55054-0_20.

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Fridman, Alexei M., and Nikolai N. Gorkavyi. "Observational Data." In Astronomy and Astrophysics Library, 21–57. Berlin, Heidelberg: Springer Berlin Heidelberg, 1999. http://dx.doi.org/10.1007/978-3-662-03918-2_2.

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Rohlfs, K., and T. L. Wilson. "Observational Methods." In Astronomy and Astrophysics Library, 166–91. Berlin, Heidelberg: Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-05394-2_7.

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Maccacaro, Tommaso, Suzanne Romaine, and Jurgen H. M. M. Schmitt. "Logn-Logs Slope Determination in Imaging X-ray Astronomy." In Observational Cosmology, 597–99. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3853-3_62.

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Arp, Halton. "Observational Problems in Extragalactic Astronomy." In Highlights of Astronomy, 43–62. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2828-5_3.

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Steele, John M. "Babylonian Observational and Predictive Astronomy." In Handbook of Archaeoastronomy and Ethnoastronomy, 1855–62. New York, NY: Springer New York, 2014. http://dx.doi.org/10.1007/978-1-4614-6141-8_191.

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Aerts, C., J. Christensen-Dalsgaard, and D. W. Kurtz. "Observational Techniques for Asteroseismology." In Astronomy and Astrophysics Library, 295–335. Dordrecht: Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-5803-5_4.

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Streszczenia konferencji na temat "Observational astronomy"

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Cline, David. "OBSERVATIONAL NEUTRINO ASTRONOMY." In Workshop on Extra Solar Neutrino Astronomy. WORLD SCIENTIFIC, 1988. http://dx.doi.org/10.1142/9789814541411.

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Primack, Joel R. "Observational Gamma-ray Cosmology." In HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP, 2005. http://dx.doi.org/10.1063/1.1878394.

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Halzen, Francis. "High-Energy Neutrino Astronomy." In THE NEW COSMOLOGY: Conference on Strings and Cosmology; The Mitchell Symposium on Observational Cosmology. AIP, 2004. http://dx.doi.org/10.1063/1.1848331.

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Lee, Joong Y., Donald Figer, Elizabeth Corrales, Jonathan Getty, and Lynn Mears. "HgCdTe detectors grown on silicon substrates for observational astronomy." In High Energy, Optical, and Infrared Detectors for Astronomy VIII, edited by Andrew D. Holland and James Beletic. SPIE, 2018. http://dx.doi.org/10.1117/12.2313401.

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Kaifu, Norio. "Rapid Progress and Limitation of Observational Astronomy in Japan." In Accelerating the Rate of Astronomical Discovery. Trieste, Italy: Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.099.0003.

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Cramer, Claire E., Steven W. Brown, Keith R. Lykke, John T. Woodward, Stephen Bailey, David J. Schlegel, Adam S. Bolton, et al. "Tunable laser techniques for improving the precision of observational astronomy." In SPIE Astronomical Telescopes + Instrumentation, edited by Ramón Navarro, Colin R. Cunningham, and Eric Prieto. SPIE, 2012. http://dx.doi.org/10.1117/12.925198.

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Baryshev, Yu V., and S. A. Oschepkov. "Gravitation theory in multimessenger astronomy II: crucial observational tests based on GW and optical observations." In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52285.

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van der Klis, M. "Kilohertz quasi-periodic oscillations-observational overview." In X-RAY ASTRONOMY: Stellar Endpoints,AGN, and the Diffuse X-ray Background. AIP, 2001. http://dx.doi.org/10.1063/1.1434653.

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Marchis, Franck, Paul G. Kalas, Marshall D. Perrin, Quinn M. Konopacky, Dmitry Savransky, Bruce Macintosh, Christian Marois, and James R. Graham. "Large collaboration in observational astronomy: the Gemini Planet Imager exoplanet survey case." In SPIE Astronomical Telescopes + Instrumentation, edited by Alison B. Peck, Robert L. Seaman, and Chris R. Benn. SPIE, 2016. http://dx.doi.org/10.1117/12.2233313.

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Perivolaropoulos, L. "Accelerating Universe: Observational Status and Theoretical Implications." In RECENT ADVANCES IN ASTRONOMY AND ASTROPHYSICS: 7th International Conference of the Hellenic Astronomical Society. AIP, 2006. http://dx.doi.org/10.1063/1.2348048.

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Raporty organizacyjne na temat "Observational astronomy"

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Kleinmann, Susan G. Observational Study and Analysis of Point Sources Found by the Infrared Astronomy Satellite. Fort Belvoir, VA: Defense Technical Information Center, April 1991. http://dx.doi.org/10.21236/ada248416.

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Helfand, David J. A Program of Ground-Based Astronomy to Complement Einstein Observations. Fort Belvoir, VA: Defense Technical Information Center, December 1986. http://dx.doi.org/10.21236/ada179331.

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Zilberman, Mark. Methods to Test the “Dimming Effect” Produced by a Decrease in the Number of Photons Received from Receding Light Sources. Intellectual Archive, November 2020. http://dx.doi.org/10.32370/iaj.2437.

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The hypothetical “Dimming Effect” describes the change of the number of photons arriving from a moving light source per unit of time. In non-relativistic systems, the “Dimming effect” may occur due to the growing distance of light sources moving away from the receiver. This means that due to the growing distance, the photons continuously require more time to reach the receiver, which reduces the number of received photons per time unit compared to the number of emitted photons. Understandably, the proposed “Dimming effect” must be tested (confirmed or rejected) through observations. a. This ar

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