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Title: AN OFF-AXIS RELATIVISTIC JET MODEL FOR THE TYPE Ic SUPERNOVA SN 2007gr

Journal Article · · Astrophysical Journal
;  [1];  [2]
  1. Department of Astronomy, Nanjing University, Nanjing 210093 (China)
  2. Yukawa Institute for Theoretical Physics, Oiwake-cho, Kitashirakawa, Sakyo-ku, Kyoto 606-8502 (Japan)

We propose an off-axis relativistic jet model for the Type Ic supernova SN 2007gr. Most of the energy ({approx}2 x 10{sup 51} erg) in the explosion is contained in non-relativistic ejecta which produces the supernova (SN). The optical emission comes from the decay process of {sup 56}Ni synthesized in the bulk SN ejecta. Only very little energy ({approx}10{sup 48} erg) is contained in the relativistic jet with initial velocity about 0.94 times the speed of light. The radio and X-ray emission comes from this relativistic jet. With some typical parameters of a Wolf-Rayet star (progenitor of Type Ic SN), i.e., the mass-loss rate M-dot =1.0x10{sup -5} M{sub sun} yr{sup -1} and the wind velocity v{sub w} = 1.5 x 10{sup 3} km s{sup -1} together with an observing angle of {theta}{sub obs} = 63.{sup 0}3, we can obtain multiband light curves that fit the observations well. All the observed data are consistent with our model. Thus, we conclude that SN 2007gr contains a weak relativistic jet and we observe the jet from off-axis.

OSTI ID:
21576581
Journal Information:
Astrophysical Journal, Vol. 735, Issue 1; Other Information: DOI: 10.1088/0004-637X/735/1/3; ISSN 0004-637X
Country of Publication:
United States
Language:
English