Margutti 2007 spectrum of GRB 060904B

主要内容:
Maybe a Nickel line.

精彩摘抄:


文章信息:

arXiv:0712.1412 [ps, pdf, other]

Title: Anomalous X-Ray emission in GRB060904B: a Nickel line?

Authors: R. Margutti, A. Moretti, F. Pasotti, S. Campana, G. Chincarini, S. Covino, C. Guidorzi, P. Romano, G. Tagliaferri

Comments: Accepted by A&A

Subjects: Astrophysics (astro-ph)

The detection of an extra component in GRB060904B X-ray spectra in addition to the standard single power-law behaviour has recently been reported in the literature. This component can be fit with different models; in particular the addition of a spectral line provides the best representation.In this paper we investigate the physical properties that the surrounding medium must have in order to produce a spectral feature that can explain the detected emission. We analyse and discuss how and if the detected spectral excess fits in different theoretical models developed to explain the nature of line emission during the afterglow phase of Gamma-Ray Bursts (GRBs). Trasmission and reflection models have been considered. Given the high value (>>1) of the Thomson optical depth, the emission is likely to arise in a reflection scenario. Within reflection models, the external reflection geometry fails to predict the observed luminosity. On the contrary, the detected feature can be explained in a funnel scenario with typical opening angle theta of 5 degrees, Nickel mass of the order of 0.1 M_o and T=10^6 K. For theta=20 degrees, assuming the reprocessing material to be the SN shell, the detected emission implies a Nickel mass of 0.4 M_o at T=10^7 K and a metallicity 10 times the solar value. If the giant X-ray flare that dominates the early XRT light curve is identified with the ionizing source, the SN expansion began 3000 s before the GRB event.