主要内容:
GRB 980425的暴本身的流量很低,一种解释是偏轴观测。如果这样的话,在一年以后的射电辐射应该会很亮(就像GRB 970508, (970508的晚期射电很亮吗?它被确认是一个偏轴观测的暴吗?))。不过实际射电观测SN 1998bw比预计的流量低三个量级,作者归结为环境的影响。
同样建议对近处的超新星的射电进行普查。
精彩摘抄:
文章信息:
Title: |
| The Nature of GRB 980425 and the Search for Off-Axis Gamma-Ray Burst Signatures in Nearby Type Ib/c Supernova Emission |
Authors: |
| Waxman, Eli |
Publication: |
| The Astrophysical Journal, Volume 602, Issue 2, pp. 886-891. (ApJ Homepage) |
Publication Date: |
| 02/2004 |
Bibliographic Code: |
| 2004ApJ...602..886W |
Abstract
The identification of Type
Ib/c supernovae (SNe
Ib/c) as gamma-ray burst (GRB) progenitors is motivated by the association of GRB 980425 with SN 1998bw and of GRB 030329 with SN 2003dh. While the gamma-ray luminosity of GRB 030329 was typical to cosmological GRBs, the luminosity of the nearby (40 Mpc) GRB 980425 was ~5 orders of magnitude lower. The large luminosity difference is commonly explained by hypothesizing either that SNe
Ib/c produce two different classes of GRBs or that GRB 980425 was a typical cosmological GRB jet viewed off-axis. In the latter scenario, strong
radio emission, L
ν~10
30ν
-1/210GHz ergs s
-1 Hz
-1, is expected at ~1 yr delay as a result of jet deceleration to subrelativistic speed, as observed from GRB 970508. The
radio luminosity of SN 1998bw was 3 orders of magnitude lower than this value. We show that the low
radio flux may be consistent with the off-axis jet interpretation, if the density of the wind surrounding the progenitor is lower than typically expected, m≡(M/10
-5M
solaryr
-1)/(v
w/10
3kms
-1)~=0.1 instead of m>~1. The lower value of m is consistent with the observed
radio emission from the SN shock driven into the wind. This interpretation predicts transition to subrelativistic expansion at ~10 yr delay, with current ~1 mJy 10 GHz flux and m
V~23 optical flux, and with ~10 mas angular source size. It also implies that in order to search for the signature of off-axis GRBs associated with nearby SNe
Ib/c, follow-up observations should be carried out on a multiyear timescale.
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