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標題: Titlebook: Supernovae; Albert G. Petschek Book 1990 Springer-Verlag New York Inc. 1990 Supernova.astronomy.astrophysics.cosmology.gravitation.gravity [打印本頁]

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書目名稱Supernovae影響因子(影響力)




書目名稱Supernovae影響因子(影響力)學科排名




書目名稱Supernovae網(wǎng)絡公開度




書目名稱Supernovae網(wǎng)絡公開度學科排名




書目名稱Supernovae被引頻次




書目名稱Supernovae被引頻次學科排名




書目名稱Supernovae年度引用




書目名稱Supernovae年度引用學科排名




書目名稱Supernovae讀者反饋




書目名稱Supernovae讀者反饋學科排名





作者: colony    時間: 2025-3-21 20:28
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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作者: paleolithic    時間: 2025-3-22 14:55
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
作者: 說明    時間: 2025-3-22 20:57

作者: 中子    時間: 2025-3-22 23:54
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
作者: 鋼盔    時間: 2025-3-23 03:05
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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作者: CREST    時間: 2025-3-23 09:56

作者: 南極    時間: 2025-3-23 14:31
Jerry Cooperstein,Edward A. Baronon and tables of rotational and centrifugal distortion constants of asymmetric-top molecules, i.e. data which roughly specifies the frequencies of the rotational transitions of these types of rotors.978-3-540-49398-3Series ISSN 1615-1844 Series E-ISSN 1616-9522
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Ronald W. Mayleon and tables of rotational and centrifugal distortion constants of asymmetric-top molecules, i.e. data which roughly specifies the frequencies of the rotational transitions of these types of rotors.978-3-540-49398-3Series ISSN 1615-1844 Series E-ISSN 1616-9522
作者: 積習已深    時間: 2025-3-23 22:45

作者: 玩忽職守    時間: 2025-3-24 05:46

作者: fidelity    時間: 2025-3-24 09:38

作者: 驚奇    時間: 2025-3-24 10:40

作者: Vulnerable    時間: 2025-3-24 17:43

作者: SLING    時間: 2025-3-24 19:35
Gamma-Rays and X-Rays from Supernovae,There are three distinct phases in a supernova when γ-rays and X-rays may be expected to be produced:
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978-1-4612-7951-8Springer-Verlag New York Inc. 1990
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Classification of Supernovae,rtance of late-time spectra. Other recent discussions of supernova classifications may be found in the chapter by Branch in this volume and by Filippenko (1989). Porter and Filippenko (1987) have summarized the observed properties of SN Ib events.
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作者: INTER    時間: 2025-3-25 17:19
0941-7834 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 the
作者: Preamble    時間: 2025-3-25 22:30
Classification of Supernovae,every supernova is unique in some aspect. There have certainly been a number of interesting surprises in the last few years for a field that is nearly 50 years old. In this chapter we give an updated summary of supernova spectral classifications, emphasizing recently introduced subtypes and the impo
作者: 芳香一點    時間: 2025-3-26 02:36
Spectra of Supernovae,e unattainable information about the physical conditions and composition of the radiation source. But the spectra of supernovae resisted interpretation for a very long time. The outstanding obstacle was the great characteristic width of the spectral features150—300 ?—corresponding to Doppler broaden
作者: 脖子    時間: 2025-3-26 08:09

作者: 粗魯性質(zhì)    時間: 2025-3-26 09:30
Radio Supernovae,ange in the electromagnetic spectrum. However, until recently the only detected radio emission associated with supernovae has been from pulsars, the spinning condensed remains of the stellar explosions, and from supernova remnants (SNR). The SNRs arise either from the interaction of the supernova ej
作者: Onerous    時間: 2025-3-26 15:15
Interaction of Supernovae with Circumstellar Matter,onary status of the star. The region around a star that is modified by these processes is referred to as the circumstellar medium. In addition to mass loss from a single star, mass transfer and mass loss in a binary system may play a role in determining the circumstellar environment.
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作者: 得罪    時間: 2025-3-27 03:52
Supernovae: The Direct Mechanism and the Equation of State,ed repeatedly, yet both remain. The first model is called the “direct” or “prompt” mechanism, and is the simpler of the two. Here stellar collapse is followed by a hydrodynamical rebound of the inner core, unleashed when the stiffness of nuclear matter puts a halt to further implosion. The bounce of
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作者: 故意    時間: 2025-3-27 14:39
Supernova Light Curves,detected a third of the way across the observable universe. This review summarizes recent work that uses the supernova light curve, the plot of luminosity versus time, to help derive a picture of supernova explosions and to explore the dimensions of the universe.
作者: 繁榮地區(qū)    時間: 2025-3-27 18:36
Radio Supernovae,ears for the level of radio emission to build up. Pulsars may possibly be radio emitters at an earlier age, but it is unlikely that their radio radiation can escape through the ejected supernova envelope during the first few decades.
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作者: 慢慢流出    時間: 2025-3-28 19:59

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