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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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樓主: STRI
21#
發(fā)表于 2025-3-25 03:41:09 | 只看該作者
22#
發(fā)表于 2025-3-25 09:51:15 | 只看該作者
23#
發(fā)表于 2025-3-25 12:03:58 | 只看該作者
24#
發(fā)表于 2025-3-25 19:44:43 | 只看該作者
25#
發(fā)表于 2025-3-25 22:32:57 | 只看該作者
26#
發(fā)表于 2025-3-26 03:11:03 | 只看該作者
Conservation and Efficiency Issues,h (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.
27#
發(fā)表于 2025-3-26 06:44:38 | 只看該作者
Conference proceedings 20051st editionGRB 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
28#
發(fā)表于 2025-3-26 09:36:45 | 只看該作者
29#
發(fā)表于 2025-3-26 15:26:57 | 只看該作者
Conservation and Efficiency Issues,, τT ≥ 2.5 during first month, its density (. ~ 10. cm.) and radial extent, ~ (4–5)×10. cm. The plateau-like SN light curve, which we reproduce by a hydrodynamical model, is powered by a combination of internal energy leakage after the explosion of an extended presupernova (~ 10. cm) and subsequent
30#
發(fā)表于 2025-3-26 18:25:52 | 只看該作者
SN 1994W: Evidence of Explosive Mass Ejection a Few Years Before Explosion, τT ≥ 2.5 during first month, its density (. ~ 10. cm.) and radial extent, ~ (4–5)×10. cm. The plateau-like SN light curve, which we reproduce by a hydrodynamical model, is powered by a combination of internal energy leakage after the explosion of an extended presupernova (~ 10. cm) and subsequent
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