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Titlebook: Stellar Atmospheres: Beyond Classical Models; L. Crivellari,I. Hubeny,D. G. Hummer Book 1991 Springer Science+Business Media Dordrecht 199

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发表于 2025-3-21 16:54:53 | 显示全部楼层 |阅读模式
书目名称Stellar Atmospheres: Beyond Classical Models
编辑L. Crivellari,I. Hubeny,D. G. Hummer
视频video
丛书名称Nato Science Series C:
图书封面Titlebook: Stellar Atmospheres: Beyond Classical Models;  L. Crivellari,I. Hubeny,D. G. Hummer Book 1991 Springer Science+Business Media Dordrecht 199
描述The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the internal structure and evolution of stars. Moreover, improvements in our knowledge of the chemical composition of stars is shedding new light on the chemical evolution of galaxies and of the Universe as a whole. Because the outer layers of stars are among the best-understood astrophysical objects, the theory of stellar atmospheres plays an important role in the study of many other types of objects. These include planetary nebulae, H II regions, interstellar matter, and objects of interest in high-energy astrophysics, such as accretion disks (close binaries, dwarf novae, cataclysmic variables, quasars, active galactic nuclei), pulsar magnetospheres, and Seyfert galaxies. Finally, as stars provide a laboratory in which plasmas can be studied under more extreme conditions than on earth, the study of stellar atmospheres has strong connections with modern physics. Astronomical observations provide
出版日期Book 1991
关键词Accretion; Galaxy; LOPES; Quasar; astrophysics; galaxies; interstellar matter; magnetosphere; neutron star; q
版次1
doihttps://doi.org/10.1007/978-94-011-3554-2
isbn_softcover978-94-010-5574-1
isbn_ebook978-94-011-3554-2Series ISSN 1389-2185
issn_series 1389-2185
copyrightSpringer Science+Business Media Dordrecht 1991
The information of publication is updating

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