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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
51#
發(fā)表于 2025-3-30 12:08:37 | 只看該作者
Radio Supernovaectured circumstellar medium (CSM) and modeling of the radio light curves allows estimation of the physical conditions in this medium. CSM structures, properties of the presupernova system, and the evolution of the system in the last stages before explosion can then be derived.
52#
發(fā)表于 2025-3-30 12:46:13 | 只看該作者
Torture: The Catastrophe of a BondWe present a selection of our VLBI images of SN 1993J, along with our latest results on its expansion and its shell structure.
53#
發(fā)表于 2025-3-30 20:35:29 | 只看該作者
Translating Trauma, Witnessing SurvivalI describe and interpret observations of the rapidly developing impact of the debris of SN1987A with its circumstellar ring.
54#
發(fā)表于 2025-3-30 22:03:51 | 只看該作者
The a-Number of Hyperelliptic Curves,The high resolution obtained through the use of VLBI gives an unique opportunity to directly observe the interaction of an expanding radio supernova with its surrounding medium. We present here results from our VLBI observations of the young supernovae SN 1979C, SN 1986J, and SN 2001gd.
55#
發(fā)表于 2025-3-31 03:53:41 | 只看該作者
Nine Years of VLBI Imaging of Supernova 1993JWe present a selection of our VLBI images of SN 1993J, along with our latest results on its expansion and its shell structure.
56#
發(fā)表于 2025-3-31 05:12:51 | 只看該作者
Supernova 1987A: The Birth of a Supernova RemnantI describe and interpret observations of the rapidly developing impact of the debris of SN1987A with its circumstellar ring.
57#
發(fā)表于 2025-3-31 10:40:39 | 只看該作者
58#
發(fā)表于 2025-3-31 16:05:05 | 只看該作者
Juan-María Marcaide,Kurt W. WeilerIncludes supplementary material:
59#
發(fā)表于 2025-3-31 21:34:24 | 只看該作者
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60#
發(fā)表于 2025-3-31 21:44:23 | 只看該作者
Translating Trauma, Witnessing Survivalonly a few days after explosion, by our group with the Very Large Array at a number of radio frequencies, as well as by other groups. As a result, it is among the best-studied radio supernovae. The observed synchrotron radio emission is thought to arise from the interaction of the SN shock with the
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