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Titlebook: Supernovae; Albert G. Petschek Book 1990 Springer-Verlag New York Inc. 1990 Supernova.astronomy.astrophysics.cosmology.gravitation.gravity

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發(fā)表于 2025-3-21 16:04:42 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Supernovae
編輯Albert G. Petschek
視頻videohttp://file.papertrans.cn/882/881890/881890.mp4
叢書名稱Astronomy and Astrophysics Library
圖書封面Titlebook: Supernovae;  Albert G. Petschek Book 1990 Springer-Verlag New York Inc. 1990 Supernova.astronomy.astrophysics.cosmology.gravitation.gravity
描述For millennia mankind has watched as the heavens move in their stately progression from night to night and from year to year, presaging with their changes the changing seasons. The sun, the moon, and the planets move in what appears to be an unchanging firmament, except occasionally when a new "star" appears. Among the new stars there are comets, novae, and finally supernovae, the subject of this book. Superstitious mankind regarded these events as significant portents and recorded them carefully so that we have records of supernovae that may reach back as far as 1300 B. C. (Clark and Stephenson, 1977; Murdin and Murdin, 1985). The Cygnus Loop, believed to be a 15,000-year-old supernova remnant at a distance of only 800 pc (Chevalier and Seward, 1988), must have awed our ancestors. Tycho‘s supernova of 1572, at a distance of 2500 pc, had a magnitude of -4. 0, comparable to Venus at its brightest, and Kepler‘s supernova of 1604 had a magnitude of - 3 or so. Thus the Cygnus Loop supernova might have had a magnitude of - 6 or so, and should have been readily visible in daytime. A supernova in Vela, about 8000 B. C. was comparably close, as was SN 1006, whose magnitude may have been -9
出版日期Book 1990
關(guān)鍵詞Supernova; astronomy; astrophysics; cosmology; gravitation; gravity; neutron star; spectroscopy
版次1
doihttps://doi.org/10.1007/978-1-4612-3286-5
isbn_softcover978-1-4612-7951-8
isbn_ebook978-1-4612-3286-5Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag New York Inc. 1990
The information of publication is updating

書目名稱Supernovae影響因子(影響力)




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書目名稱Supernovae網(wǎng)絡(luò)公開度學(xué)科排名




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0941-7834 o, and should have been readily visible in daytime. A supernova in Vela, about 8000 B. C. was comparably close, as was SN 1006, whose magnitude may have been -9978-1-4612-7951-8978-1-4612-3286-5Series ISSN 0941-7834 Series E-ISSN 2196-9698
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on as a function of mass in the Hyades. It is shown that the available sample of F stars is not homogeneous and is probably made of at least two sub-groups with a very different characteristic time .. of spin down. (3) pre-main sequence stars. It is suggested that electromagnetic braking begins duri
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Robert P. Kirshner Studien- richtung "Allgemeine und Theoretische Elektrotechnik" Studierende ein Hoch- schuldip1om erwerben k?nnen. Der wissenschaftlich Nachwuchs kann im Fachge- biet "Theoretische Elektrotechnik" promovieren und im Anschlu? dar an habili- tieren. Damit besteht hier eine einzigartige Tradition zur Q
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Peter G. Sutherlandn und damit den instation?ren Feldern zuzurechnen sind. Betrachtet man aber den in der Elektrotechnik wichtigen Fall, zeitlich langsam ver?nderlicher Felder mit Leitungsl?ngen, die viel kleiner sind als die Wellenl?ngen, so tritt bei diesen noch keine Antennenwirkung auf. Es handelt sich hier um fast ortsfest978-3-322-94071-1
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