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Titlebook: Cosmic Explosions; On the 10th Annivers Juan-María Marcaide,Kurt W. Weiler Conference proceedings 20051st edition Springer-Verlag Berlin He

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書目名稱Cosmic Explosions
副標(biāo)題On the 10th Annivers
編輯Juan-María Marcaide,Kurt W. Weiler
視頻videohttp://file.papertrans.cn/239/238877/238877.mp4
概述Includes supplementary material:
圖書封面Titlebook: Cosmic Explosions; On the 10th Annivers Juan-María Marcaide,Kurt W. Weiler Conference proceedings 20051st edition Springer-Verlag Berlin He
描述Supernovae are among the most energetic phenomena in the Universe and - lated to almost all aspects of modern astrophysics including starburst gal- ies, cosmic ray acceleration, neutron star and black hole formation, nuc- osynthesis and ISM chemical enrichment, energy input to the ISM, cosmic distance scale determination, dark energy related cosmological acceleration, gamma-ray bursts, extra-solar system neutrino burst detection, gravity wave generation, and many more. Additionally, the past 15 years have been p- ticularly productive with many new results and new understanding due in particular to the closest SN in 400 years in SN 1987A in the Large M- ellanic Cloud, and the unusually bright and close SN 1993J and SN 1994I in the nearby galaxies M81 and M51, respectively. In addition, the disc- ery of the ?-ray burst GRB 980425 and its related supernova SN 1998bw, and the con?rmation of GRB 030329/SN 2003dh, tied the study of SNe and GRBs inextricably together. With the many developments since the last - jor supernova meeting in La Serena, Chile in 1997, we felt that it was an appropriate time to bring together experts and students interested in the subject for a meeting where SN a
出版日期Conference proceedings 20051st edition
關(guān)鍵詞Cosmology; Redshift; Universe; gamma-ray bursts; stellar candles; supernovae
版次1
doihttps://doi.org/10.1007/b137830
isbn_softcover978-3-642-42187-7
isbn_ebook978-3-540-26633-4
copyrightSpringer-Verlag Berlin Heidelberg 2005
The information of publication is updating

書目名稱Cosmic Explosions影響因子(影響力)




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Low Frequency Radio and X-ray Properties of Core-Collapse Supernovaeh (GRB030329) obtained with combined GMRT and VLA data. We report on the low frequency radio monitoring of SN 1995N and our objectives of distinguishing between competing models of X-ray emission from this SN and the nature of its progenitor by X-ray spectroscopy. Radio studies on SN 2001gd, SN 2001ig and SN 2002hh are mentioned.
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Torture: The Catastrophe of a Bond modeled with two different slopes. The swept-up mass estimate at an age of 3159 days (~0.4 M.), comparable to the low-mass envelope, favors a binary scenario. The observed spectral index of SN 1993J has slowly flattened since age 1000 days onward (α has changed from ?1 to ?0.67 at an age of 2820 days).
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Translating Trauma, Witnessing Survivale fully-developed dataset, and compare this to our earlier characterization made in 1994. SN 1993J has also been a target of X-ray satellites, and we briefly discuss the nature of the X-ray emission and, together with the radio emission, describe the implications for the nature of the SN’s progenitor.
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發(fā)表于 2025-3-23 08:51:49 | 只看該作者
Torture: The Catastrophe of a Bond of SN 1993J further away from us is strongly or totally absorbed. We describe the GFD method and present our findings about the emission structure of the shell. We also present the expansion of SN 1993J based on a method complementary to GFD, which will be described elsewhere.
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