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Titlebook: Supernovae and Gamma-Ray Bursters; Kurt W. Weiler Book 2003 Springer-Verlag Berlin Heidelberg 2003 Cosmology.gamma-ray bursts.standard can

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书目名称Supernovae and Gamma-Ray Bursters
编辑Kurt W. Weiler
视频video
概述Bridges the gap between standard textbook material and the forefront of research.Includes supplementary material:
丛书名称Lecture Notes in Physics
图书封面Titlebook: Supernovae and Gamma-Ray Bursters;  Kurt W. Weiler Book 2003 Springer-Verlag Berlin Heidelberg 2003 Cosmology.gamma-ray bursts.standard can
描述Since the dawn of mankind, observers of the sky have wondered at the sudden appearance of new stars on the seemingly unchanging heavens and, for at least 2000 years, have recorded these phenomena in their annals and archives. Even in more modern times, since the discovery of SN1885A in S Andromeda which ?gured in the important “island universe” discussions of the 1920’s, the puzzle of supernovae (SNe) has played an important role in astrophysics. Only with the seminal work of Fritz Zwicky and Walter Baade in the 1930’s did we begin to understand the di?erences between novae and SNe and the importance of SNe as the fonts of energy for the interstellar medium and as drivers of chemical evolution in galaxies. As recently as the 1940’s and 1950’s the early days of radio astronomy were heavily in?uenced by the familiar names of Cassiopeia A and Taurus A, two young supernova remnants, and two Nobel prizes have been awarded for discovery and study of a related phenomenon, pulsars. In spite of the great age of the study of SNe, since at least the Chinese records of SN185and probably earlier, the ?eld is, in fact, very young having only attracted a large devoted following since the spectacu
出版日期Book 2003
关键词Cosmology; gamma-ray bursts; standard candles; stellar; supernovae
版次1
doihttps://doi.org/10.1007/3-540-45863-8
isbn_softcover978-3-642-07893-4
isbn_ebook978-3-540-45863-0Series ISSN 0075-8450 Series E-ISSN 1616-6361
issn_series 0075-8450
copyrightSpringer-Verlag Berlin Heidelberg 2003
The information of publication is updating

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Measuring Cosmology with Supernovaeears large enough to challenge these current results. Future experiments are planned to better character ize the equation of state of the dark energy leading to the observed acceleration by observing hundreds or even thousands of objects. These experiments will need to carefully control systematic e
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SN1998bw and Hypernovaeution of the radio light curves suggest the existence of a relativistic blast wave in SN1998bw, which might be related to the .-ray burst directly or indirectly. Several other several hypernova candidates have been discovered or reinterpreted since SN1998bw. The unusual properties of these objects m
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Lecture Notes in Physicshttp://image.papertrans.cn/t/image/881893.jpg
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