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Relevant bibliographies by topics / Fundamental astronomy and astrophysics

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Academic literature on the topic 'Fundamental astronomy and astrophysics'

Author: Grafiati

Published: 17 September 2021

Last updated: 18 July 2025

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Journal articles on the topic "Fundamental astronomy and astrophysics"

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STAMATIKOS, MICHAEL. "GRB ASTROPHYSICS IN THE SWIFT ERA AND BEYOND." International Journal of Modern Physics D 18, no. 10 (2009): 1567–70. http://dx.doi.org/10.1142/s0218271809015631.

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Gamma-ray Bursts (GRBs) are relativistic cosmological beacons of transient high energy radiation whose afterglows span the electromagnetic spectrum. Theoretical expectations of correlated neutrino emission position GRBs at an astrophysical nexus for a metamorphosis in our understanding of the Cosmos. This new dawn in the era of experimental (particle) astrophysics and cosmology is afforded by current facilities enabling the novel astronomy of high energy neutrinos, in concert with unprecedented electromagnetic coverage. In that regard, GRBs represent a compelling scientific theme that may faci

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Fukushima, Toshio, Jan Vondrak, Nicole Capitaine, et al. "Division I: Fundamental Astronomy." Proceedings of the International Astronomical Union 1, T26A (2005): 1. http://dx.doi.org/10.1017/s174392130700107x.

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IAU Division I includes Commission 4 (Ephemerides), Commission 7 (Celestial Mechanics and Dynamical Astronomy), Commission 8 (Astrometry), Commission 19 (Rotation of the Earth) and Commission 31 (Time). The Division has in addition five Working Groups on, respectively, Future Development of Ground-Based Astrometry, Nomenclature for Fundamental Astrometry, Definition of Coordinated Universal Time, and Precession and the Ecliptic.

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Fukushima, Toshio, Jan Vondrák, Nicole Capitaine, et al. "DIVISION I: FUNDAMENTAL ASTRONOMY." Proceedings of the International Astronomical Union 3, T26B (2007): 71–73. http://dx.doi.org/10.1017/s1743921308023673.

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Division I provides a focus for astronomers studying a wide range of problems related to fundamental physical phenomena such as time, the inertial reference frame, positions and proper motions of celestial objects, and precise dynamical computation of the motions of bodies in stellar or planetary systems in the Universe.

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Vondrák, Jan, and Dennis D. McCarthy. "DIVISION I - Fundamental Astronomy." Proceedings of the International Astronomical Union 3, T26B (2007): 284–305. http://dx.doi.org/10.1017/s1743921308024368.

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Aleksander Brzezinski, P-C19 (Poland), Joseph A. Burns, P-C7 (USA), Pascale Defraigne, P-C31 (Belgium), Dafydd Wyn Evans, VP-C8 (UK) Toshio Fukushima, P-C4, PP (Japan), George H. Kaplan, VP-C4 (USA), Sergei A. Klioner, P-C52 (Germany), Zoran Knezevic, VP-C7 (Serbia) Irina I. Kumkova, P-C8 (Russia), Chopo Ma, VP-C19 (USA), Richard N. Manchester, VP-C31 (Australia), and Gérard Petit, VP-C52 (France)

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Vondrák, Jan, Dennis D. McCarthy, Toshio Fukushima, et al. "DIVISION I: FUNDAMENTAL ASTRONOMY." Proceedings of the International Astronomical Union 4, T27A (2008): 1–4. http://dx.doi.org/10.1017/s1743921308025222.

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Division I provides a focus for astronomers studying a wide range of problems related to fundamental physical phenomena such as time, the inertial reference frame, positions and proper motions of celestial objects and precise dynamical computation of the motions of bodies in stellar or planetary systems in the Universe.

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Lépine-Szily, Alinka, and Pierre Descouvemont. "Nuclear astrophysics: nucleosynthesis in the Universe." International Journal of Astrobiology 11, no. 4 (2012): 243–50. http://dx.doi.org/10.1017/s1473550412000158.

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AbstractNuclear astrophysics is a relatively young science; it is about half a century old. It is a multidisciplinary subject, since it combines nuclear physics with astrophysics and observations in astronomy. It also addresses fundamental issues in astrobiology through the formation of elements, in particular those required for a carbon-based life. In this paper, a rapid overview of nucleosynthesis is given, mainly from the point of view of nuclear physics. A short historical introduction is followed by the definition of the relevant nuclear parameters, such as nuclear reaction cross sections

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Saxena, P. P. "Teaching of Astronomy in India: With Special Reference to Teaching of Astronomy at Lucknow University." International Astronomical Union Colloquium 105 (1990): 394–97. http://dx.doi.org/10.1017/s0252921100087352.

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Modern astronomy started in India when an astronomical observatory was founded in Madras as early as 1786 by the East India Company and to which the Indian Institute of Astrophysics traces its origin. There are, however, records of astronomical observations taken through a telescope from Pondicherry that elucidate the double-star nature of Alpha-Centauri as early as in 1689. Since then many more research centers in astronomy have been established. Today, institutions like the Indian Institute of Astrophysics (Bangalore), the Raman Research Institute (Bangalore), the Center of Advanced Study in

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de Castro, Ana I. Gómez, Willem Wamsteker, Martin Barstow, et al. "Fundamental Problems in Astrophysics." Astrophysics and Space Science 303, no. 1-4 (2006): 133–45. http://dx.doi.org/10.1007/s10509-006-9057-4.

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Onuora, Lesley I. "Astronomy in Nigeria." Highlights of Astronomy 10 (1995): 666–67. http://dx.doi.org/10.1017/s1539299600012491.

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One major problem in Africa in general is to convince governments and agencies that astronomy is relevant to Africa. Attention has been focussed on technology transfer, neglecting science and research. This attitude encourages the continued dependence on industrialized countries.In Nigeria there has been some success in projecting the idea that Space Science does not just mean remote sensing, but that basic space science, i.e. astronomy and astrophysics, cosmology, planetary science etc. is important and necessary. Evidence of this is that Nigeria’s expert committee on space policy recommended

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Klioner, Sergei A., Gérard Petit, Victor A. Brumberg, et al. "COMMISSION 52: RELATIVITY IN FUNDAMENTAL ASTRONOMY." Proceedings of the International Astronomical Union 4, T27A (2008): 55–59. http://dx.doi.org/10.1017/s1743921308025295.

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The tremendous progress in technology which we have witnessed during the last 30 years has led to enormous improvements of observational accuracy in all disciplines of fundamental astronomy. Relativity has been becoming increasingly important for modeling and interpretation of high accuracy astronomical observations during at least these 30 years. It is clear that for current accuracy requirements astronomical problems have to be formulated within the framework of General Relativity Theory. Many high-precision astronomical techniques have already required the application of relativistic effect

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Dissertations / Theses on the topic "Fundamental astronomy and astrophysics"

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Davis, Adam N. "Astrophysical Constraints on Fundamental Parameters in Physics and Astronomy." Case Western Reserve University School of Graduate Studies / OhioLINK, 2004. http://rave.ohiolink.edu/etdc/view?acc_num=case1098973318.

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Czekala, Ian. "The Fundamental Properties of Young Stars." Thesis, Harvard University, 2016. http://nrs.harvard.edu/urn-3:HUL.InstRepos:33493279.

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Accurate knowledge of the fundamental properties of stars--mass, temperature, and luminosity--is key to our understanding of stellar evolution. In particular, empirical measurements of stellar mass are difficult to make and are generally limited to stars that dynamically interact with a companion (e.g., eclipsing or astrometric binaries), a precious but ultimately small sample. We developed a technique that uses the rotation of the protoplanetary disk--a consequence of the star formation process still present around many pre-main sequence stars--to measure the stellar mass. To establish the ab

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AN, JIN HYEOK. "Astrophysics from binary-lens microlensing." The Ohio State University, 2002. http://rave.ohiolink.edu/etdc/view?acc_num=osu1029254036.

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Davis, Adam N. "Astrophysical constraints on fundamental paramenters in physics and astronomy." online version, 2005. http://rave.ohiolink.edu/etdc/view?acc%5Fnum=case1098973318.

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Maccione, Luca. "High-energy astrophysics, cosmic rays and fundamental physics." Doctoral thesis, SISSA, 2008. http://hdl.handle.net/20.500.11767/4164.

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This thesis is devoted to the study of phenomenological consequences of theoretical models of Quantum Gravity. In particular, this work is focused on the study of possible violations of Lorentz invariance, which may arise if, owing to quantum gravity effects, the high-energy structure of the spacetime is different from the smooth, continuous one we are used to in our low-energy world. After a brief description of the most widely known models accounting for Lorentz invariance violations, particular focus will be given to astrophysical tests of Lorentz invariance. These are motivated by the fact

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Ryle, Wesley Thomas. "Investigation of Fundamental Black Hole Properties of AGN through Optical Variability." Digital Archive @ GSU, 2008. http://digitalarchive.gsu.edu/phy_astr_diss/25.

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Active galactic nuclei (AGN) are known to vary in brightness in all regions of the electromagnetic spectrum and over a wide range of timescales. Many methods have been utilized to transform this observed variability into meaningful information about the central engines of AGN. One such technique, adapted from time series analysis of galactic x-ray binary systems, has been used to detect a characteristic break timescale in the power density spectra of x-ray variability in Seyfert galaxies. This timescale, thought to be related to instabilities in the accretion disk, appears to scale with bla

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Pesquero, Lucas Canevarolo. "Proposta de um minicurso de Astronomia para alunos do Ensino Fundamental II." Universidade Federal de São Carlos, 2015. https://repositorio.ufscar.br/handle/ufscar/7315.

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Submitted by Izabel Franco (izabel-franco@ufscar.br) on 2016-09-20T19:10:07Z No. of bitstreams: 1 DissLCP.pdf: 1996669 bytes, checksum: 2a08a209c281476b0ab43a88b088630f (MD5)<br>Approved for entry into archive by Marina Freitas (marinapf@ufscar.br) on 2016-09-21T12:41:01Z (GMT) No. of bitstreams: 1 DissLCP.pdf: 1996669 bytes, checksum: 2a08a209c281476b0ab43a88b088630f (MD5)<br>Approved for entry into archive by Marina Freitas (marinapf@ufscar.br) on 2016-09-21T12:41:07Z (GMT) No. of bitstreams: 1 DissLCP.pdf: 1996669 bytes, checksum: 2a08a209c281476b0ab43a88b088630f (MD5)<br>Made available

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Boyajian, Tabetha Suzanne. "Sizing Up the Stars." Digital Archive @ GSU, 2009. http://digitalarchive.gsu.edu/phy_astr_diss/34.

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For the main part of this dissertation, I have executed a survey of nearby, main sequence A, F, and G-type stars with the CHARA Array, successfully measuring the angular diameters of forty-four stars to better than 4% accuracy. The results of these observations also yield empirical determinations of stellar linear radii and effective temperatures for the stars observed. In addition, these CHARA-determined temperatures, radii, and luminosities are fit to Yonsei-Yale isochrones to constrain the masses and ages of the stars. These quantities are compared to the results found in Allende Prieto & L

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Al, Moulla Khaled. "Advanced Characterization of Exoplanet Host Stars." Thesis, Uppsala universitet, Observationell astrofysik, 2020. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-414368.

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The spectroscopic determination of stellar properties is important for subsequent studies of exoplanet atmospheres. In this thesis, HARPS data for 6 exoplanet-hosting, late-type stars is processed to achieve an average signal-to-noise ratio of ~105. Together with line data, the SME tool is used to synthesize spectra and interpolate model photospheres with which chi-square minimization is performed. Fundamental parameters are derived to an overall precision of 191 K in effective temperature, 0.88 dex in surface gravity and 0.21 dex in metallicity. For 5 of the stars, the parameters are thereaft

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Neilson, Hilding R., Joseph T. McNeil, Richard Ignace, and John B. Lester. "Limb Darkening and Planetary Transits: Testing Center-to-limb Intensity Variations and Limb-darkening Directly from Model Stellar Atmospheres." Digital Commons @ East Tennessee State University, 2017. https://dc.etsu.edu/etsu-works/2684.

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The transit method, employed by Microvariability and Oscillation of Stars (MOST), Kepler, and various ground-based surveys has enabled the characterization of extrasolar planets to unprecedented precision. These results are precise enough to begin to measure planet atmosphere composition, planetary oblateness, starspots, and other phenomena at the level of a few hundred parts per million. However, these results depend on our understanding of stellar limb darkening, that is, the intensity distribution across the stellar disk that is sequentially blocked as the planet transits. Typically, stella

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Books on the topic "Fundamental astronomy and astrophysics"

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Ferreras, Ignacio. Fundamentals of Galaxy Dynamics, Formation and Evolution. UCL Press, 2019.

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ESO-CERN Symposium (2nd 1986 Garching bei München, Germany). Cosmology, astronomy and fundamental physics: Second ESO-CERN Symposium, ESO, Garching bei München, 17-21 March 1986 : proceedings. European Southern Observatory, 1986.

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R, Bedding T., Booth A. J, and Davis John, eds. Fundamental stellar properties: The interaction between observation and theory : proceedings of the 189th Symposium of the International Astronomical Union, held atthe Women's College, University of Sydney, Australia, 13-17 January 1997. Kluwer Academic, 1997.

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Symposium, International Astronomical Union. Fundamental stellar properties: The interaction between observation and theory : proceedings of the 189th Symposium of the International Astronomical Union, held at the Women's College, University of Sydney, Australia, 13-17 January 1997. Kluwer Academic, 1997.

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International Colloquium on Perspectives of High Energy Astronomy and Astrophysics (1996 Tata Institute of Fundamental Research). High energy astronomy and astrophysics: Proceedings of the International Colloquium on Perspectives of High Energy Astronomy and Astrophysics to commemorate the golden jubilee year of Tata Institute of Fundamental Research, Mumbai, India, August 12-17, 1996. Edited by Agrawal P. C, Vishwanath P. R, and Tata Institute of Fundamental Research. University Press, 1998.

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Bénédicte, Leclercq, ed. The natural laws of the universe: Understanding fundamental constants. Springer, 2008.

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Paolo, Molaro, and SpringerLink (Online service), eds. From Varying Couplings to Fundamental Physics: Proceedings of Symposium 1 of JENAM 2010. Springer-Verlag Berlin Heidelberg, 2011.

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Paula, Benaglia, Bosch Guillermo 1968-, Cappa Cristina, Niemela Virpi, and Universidad Nacional Autónoma de México. Instituto de Astronomía., eds. Massive stars: Fundamental parameters and circumstellar interactions : Cariló, Buenos Aires, Argentina, diciembre 11-14, 2006. Instituto de Astronomía, Universidad Nacional Autónoma de México, 2008.

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A, Klioner Sergei, Seidelmann P. Kenneth, and Soffel Michael H. 1953-, eds. Relativity in fundamental astronomy: Dynamics, reference frames, and data analysis : proceedings of the 261st Symposium of the International Astronomical Union held in Virginia Beach, Virginia, USA : April 27-May 1, 2009. Cambridge University Press, 2010.

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S, Roberts Morton, ed. Astronomy & astrophysics. American Association for the Advancement of Science, 1985.

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Book chapters on the topic "Fundamental astronomy and astrophysics"

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Walter, Hans G., and Ojars J. Sovers. "Fundamental Catalogues." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-57260-9_1.

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Walter, Hans G., and Ojars J. Sovers. "The Conventional Fundamental Catalogue FK5." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-57260-9_2.

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Walter, Hans G., and Ojars J. Sovers. "Fundamental Catalogues of Extragalactic Radio Sources." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-57260-9_5.

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Kramer, Michael. "Pulsar Timing - From Astrophysics to Fundamental Physics." In Reviews in Modern Astronomy. Wiley-VCH Verlag GmbH & Co. KGaA, 2008. http://dx.doi.org/10.1002/9783527622993.ch11.

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Koshiba, M. "Neutrino Astrophysics: Its Birth and Future." In Astronomy, Cosmology and Fundamental Physics. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0965-6_24.

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Walter, Hans G., and Ojars J. Sovers. "Contributions of Space Astrometry to Fundamental Catalogues." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 2000. http://dx.doi.org/10.1007/978-3-642-57260-9_3.

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Perryman, M. A. C. "The Contribution of Hipparcos to Fundamental Astronomy." In Astrophysics and Space Science Library. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0794-5_11.

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Rohlfs, Kristen. "Radio Astronomical Fundamentals." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-662-02465-2_1.

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Rohlfs, Kristen. "Line Radiation Fundamentals." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 1986. http://dx.doi.org/10.1007/978-3-662-02465-2_10.

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Rohlfs, K., and T. L. Wilson. "Radio Astronomical Fundamentals." In Astronomy and Astrophysics Library. Springer Berlin Heidelberg, 2004. http://dx.doi.org/10.1007/978-3-662-05394-2_1.

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Conference papers on the topic "Fundamental astronomy and astrophysics"

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Melnikov, V. N. "Multidimensional models, dark energy and fundamental constants." In ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology After Gamow and the 9th Gamow Summer School “Astronomy and Beyond: Astrophysics, Cosmology, Radio Astronomy, High Energy Physics and Astrobiology”. American Institute of Physics, 2010. http://dx.doi.org/10.1063/1.3292512.

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Bisnovatyi‐Kogan, G. S. "Binary Recycled Pulsar as a Laboratory for the Fundamental Physics." In ASTROPHYSICS AND COSMOLOGY AFTER GAMOW: Proceedings of the 4th Gamow International Conference on Astrophysics and Cosmology After Gamow and the 9th Gamow Summer School “Astronomy and Beyond: Astrophysics, Cosmology, Radio Astronomy, High Energy Physics and Astrobiology”. American Institute of Physics, 2010. http://dx.doi.org/10.1063/1.3292527.

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Kruk, Sandor, Oana Romocea, Eliza Casapopol, Cristian Ignat, Iuliana Bledea, and Alina Vizireanu. "Space education activities at the Romanian Science Festival." In Symposium on Space Educational Activities (SSAE). Universitat Politècnica de Catalunya, 2022. http://dx.doi.org/10.5821/conference-9788419184405.131.

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Eastern European countries, in particular Romania, offer much fewer opportunities for science and space outreach and informal science education compared to the West. Romanian Science Festival was founded in 2018 with the aim of answering questions raised by the inquisitive minds of children all over Romania. In 2019, we reached over 20,000 people with our live events: open-air science festivals, space talks and astronomical observations. During the COVID-19 pandemic, we organised 58 live webinars of over 75 hours in total, one of the largest scientific resources in the Romanian language. Moreo

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Halzen, Francis, John Learned, and Todar Stanev. "Neutrino Astronomy." In Astrophysics in Antarctica. AIP, 1990. http://dx.doi.org/10.1063/1.39028.

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Harper, D. A. "Infrared astronomy in Antarctica." In Astrophysics in Antarctica. AIP, 1990. http://dx.doi.org/10.1063/1.39022.

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Vacanti, G. "Gamma-ray astronomy at 1 TeV." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39151.

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Cherry, Michael L. "Neutrino astronomy on the moon—practical considerations." In Particle astrophysics. AIP, 1990. http://dx.doi.org/10.1063/1.39130.

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Hogan, Craig J. "Brane-world astronomy." In RELATIVISTIC ASTROPHYSICS: 20th Texas Symposium. AIP, 2001. http://dx.doi.org/10.1063/1.1419526.

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Smith, A. J. "Astrophysics with Milagro." In HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP, 2005. http://dx.doi.org/10.1063/1.1878479.

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Weeks, Trevor C. "Very high energy gamma ray astronomy." In Astrophysics in Antarctica. AIP, 1990. http://dx.doi.org/10.1063/1.38992.

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Reports on the topic "Fundamental astronomy and astrophysics"

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Harrison, Fiona, Robert Kennicutt, Julianne Dalcanton, et al. Pathways to Discovery in Astronomy and Astrophysics for the 2020s. Office of Scientific and Technical Information (OSTI), 2023. http://dx.doi.org/10.2172/2326985.

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Cortés Rodríguez, Patricio, Denise Depoortere, and Lucy Opazo Calfin. Conjunto de datos: Datasets indexed in Data Citation Index in the Astronomy and Astrophysics category, 2010-2019. Pontificia Universidad Católica de Chile, 2021. http://dx.doi.org/10.7764/datasetuc/62181.

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Malchenko, Svitlana L., Davyd V. Mykoliuk, and Arnold E. Kiv. Using interactive technologies to study the evolution of stars in astronomy classes. [б. в.], 2020. http://dx.doi.org/10.31812/123456789/3752.

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In astrophysics, a significant role is played by observations. During astronomy classes in the absence of surveillance tools interactive programmes such as an interactive programme for space objects simulation can be used as Universe Sandbox2. The aim of this work is to implement interactive programmes for effective astronomy teaching, understanding material and increasing cognitive interest. We observe the evolution of stars while using Universe Sandbox2 during the study of the topic “Evolution of stars”. Using this programme students have an opportunity to get acquainted with the existence o

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Ormand, W., P. Navratil, and S. Libby. Stellar Astrophysics and a Fundamental Description of Thermonuclear Reactions ? 04-ERD-058 Final Report. Office of Scientific and Technical Information (OSTI), 2007. http://dx.doi.org/10.2172/902351.

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Wefel, J. P., and T. G. Guzik. Nuclear interactions in high energy heavy ions and applications in astrophysics. [Dept. of Physics and Astronomy, Louisiana State Univ. , Baton Rouge]. Office of Scientific and Technical Information (OSTI), 1993. http://dx.doi.org/10.2172/6703061.

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Forest, Cary B. Feasibility Study for a Plasma Dynamo Facility to Investigate Fundamental Processes in Plasma Astrophysics. Final report. Office of Scientific and Technical Information (OSTI), 2013. http://dx.doi.org/10.2172/1093448.

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Hill, C. 21st Atomic Processes in Plasmas Conference. IAEA Nuclear Data Section, 2023. http://dx.doi.org/10.61092/iaea.csbv-dg73.

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The 21st Atomic Processes in Plasmas Meeting was held as a Technical Meeting of the IAEA from 15 – 19 May 2023. The meeting encompasses atomic plasmas across a wide range of densities and temperatures with application to astrophysics, fundamental data and modelling, fusion energy research, warm dense matter and laser-plasma interactions. 127 participants from 30 IAEA Member States registered for the event, which included 57 oral presentations and 47 posters; six tutorial lectures on atomic processes in plasmas were also included in the programme. This report provides a summary of the agenda, p

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