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Titlebook: The Early Type Stars; Anne B. Underhill Book 1966 Springer Science+Business Media Dordrecht 1966 Libration.Population.Variation.cosmic ray

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書目名稱The Early Type Stars
編輯Anne B. Underhill
視頻videohttp://file.papertrans.cn/909/908005/908005.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: The Early Type Stars;  Anne B. Underhill Book 1966 Springer Science+Business Media Dordrecht 1966 Libration.Population.Variation.cosmic ray
描述At this time when astronomers are being surprised by the discovery of objects which emit a fabulously large amount of energy, that is the quasi-stellar radio sources and the quasi-stellar galaxies, and when by the means of space vehicles X rays, gamma rays and cosmic rays are being observed to come from the depths of interstellar space, one may ask why write a book about stars. Stars seem to be almost incidental when one looks at the universe in terms of exceedingly great energies. Nevertheless, stars exist. They are accessible to study and they have not yet revealed all their secrets. This is enough to arouse interest and to cause one to try to find answers to the questions which arise. The early type stars are particularly interesting because they are spendthrift stars pouring out their energy at a great rate. But their brilliance is also their undoing. They must evolve rather quickly, on an astrophysical scale. Thus by studying these stars we are studying a population in change. The implications from the local and from the cosmological viewpoint are important if one wishes to understand the details of stellar evolution and of galactic structure. Perhaps one of the simplest reaso
出版日期Book 1966
關鍵詞Libration; Population; Variation; cosmic ray; galaxies; galaxy; star; stars; stellar evolution; universe
版次1
doihttps://doi.org/10.1007/978-94-010-3556-9
isbn_softcover978-94-010-3558-3
isbn_ebook978-94-010-3556-9Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1966
The information of publication is updating

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