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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
41#
發(fā)表于 2025-3-28 14:40:13 | 只看該作者
SN 1994W: Evidence of Explosive Mass Ejection a Few Years Before Explosionofiles are composed of three major components: (i) narrow P Cygni lines with absorption minima at ?700 km s.; (ii) broad emission lines with blue velocity at zero intensity ~ 4000 km s.; (iii) broad, smooth, extended wings most apparent in H.. These components are identified with the expanding circu
42#
發(fā)表于 2025-3-28 20:33:44 | 只看該作者
43#
發(fā)表于 2025-3-29 00:13:31 | 只看該作者
44#
發(fā)表于 2025-3-29 03:10:54 | 只看該作者
Synthetic Spectra of the Type Ia SN 2002bois one of the earliest observed SNe. An almost complete set of spectra and photometry is available from 13 days before maximum . light until a few days after. An analysis using synthetic spectra is presented, focusing on the controversial issue of the reddening of SN 2002bo.
45#
發(fā)表于 2025-3-29 09:27:36 | 只看該作者
46#
發(fā)表于 2025-3-29 14:34:24 | 只看該作者
47#
發(fā)表于 2025-3-29 18:11:50 | 只看該作者
https://doi.org/10.1007/b137830Cosmology; Redshift; Universe; gamma-ray bursts; stellar candles; supernovae
48#
發(fā)表于 2025-3-29 21:38:40 | 只看該作者
978-3-642-42187-7Springer-Verlag Berlin Heidelberg 2005
49#
發(fā)表于 2025-3-30 02:38:17 | 只看該作者
Detection of the Binary Companion to the Progenitor of SN 1993Jomponent in the spectra of SN1993J which cannot be explained by the surrounding faint blue stars. This is the first detection of the expected massive binary companion to the red supergiant progenitor and confirms that SN1993J did indeed arise in an interacting binary system.
50#
發(fā)表于 2025-3-30 07:51:49 | 只看該作者
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