Tichardson 2006 IIb, Ib, Ic光变曲线聚合

主要内容:
收集了3个IIb，11个Ib，13个Ic型超新星的光变曲线、宿主星系信息等。
其中IIb型超新星有：
1987K 1993J 1996cb
Ib型超新星有：
1954A 1983N 1984I 1984L 1990I 1991D 1998dt 1999di 1999dn 1999ex 2000H
Ic型超新星有：
1962L 1964L 1983I 1983V 1987M 1990B 1991N 1992ar 1994I 1997ef 1998bw 1999cq 2002ap

精彩摘抄:
Ic SNe

文章信息:

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· arXiv e-print (arXiv:astro-ph/0601136)

· References in the article

· Citations to the Article (22) (Citation History)

· Refereed Citations to the Article

· SIMBAD Objects (56)

· NED Objects (54)

· Also-Read Articles (Reads History)

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Title:		Absolute Magnitude Distributions and Light Curves of Stripped-Envelope Supernovae
Authors:		Richardson, Dean; Branch, David; Baron, E.
Affiliation:		AA(Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019.; Physics Department, Marquette University, Milwaukee, WI 53201.), AB(Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019.), AC(Department of Physics and Astronomy, University of Oklahoma, Norman, OK 73019.)
Publication:		The Astronomical Journal, Volume 131, Issue 4, pp. 2233-2244. (AJ Homepage)
Publication Date:		04/2006
Origin:		UCP
AJ Keywords:		Stars: Evolution, Stars: Supernovae: General
Abstract Copyright:		(c) 2006: The American Astronomical Society
DOI:		10.1086/500578
Bibliographic Code:		2006AJ....131.2233R

Abstract

The absolute visual magnitudes of three Type IIb, 11 Type Ib, and 13 Type Ic supernovae (collectively known as stripped-envelope supernovae) are studied by collecting data on the apparent magnitude, distance, and interstellar extinction of each event. Weighted and unweighted mean absolute magnitudes of the combined sample, as well as various subsets of the sample, are reported. The limited sample size and the considerable uncertainties, especially those associated with extinction in the host galaxies, prevent firm conclusions regarding differences between the absolute magnitudes of supernovae of Types Ib and Ic, and regarding the existence of separate groups of overluminous and normal-luminosity stripped-envelope supernovae. The spectroscopic characteristics of the events of the sample are considered. Three of the four overluminous events are known to have had unusual spectra. Most but not all of the normal-luminosity events have had typical spectra. The light curves of stripped-envelope supernovae are collected and compared. Because SN 1994I in M51 was very well observed, it often is regarded as the prototypical Type Ic supernova, but it has the fastest light curve in the sample. Light curves are modeled by means of a simple analytical technique that, combined with a constraint on E/M from spectroscopy, yields internally consistent values of ejected mass, kinetic energy, and nickel mass.

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