Evidence of contribution of intervening clouds to gamma-ray Burst's X-ray column density

7Citations
Citations of this article
7Readers
Mendeley users who have this article in their library.

Abstract

The origin of excess of X-ray column density with respect to optical extinction in gamma-ray bursts (GRBs) is still a puzzle. A proposed explanation of the excess is the photoelectric absorption due to the intervening clouds along a GRB's line of sight. Here, we test this scenario by using the intervening Mg II absorption as a tracer of the neutral hydrogen column density of the intervening clouds. We identify a connection between the large X-ray column density (and large column density ratio of NH,X/N H1) and large neutral hydrogen column density probed by the Mg II doublet ratio (DR). In addition, GRBs with large X-ray column density (and large ratio of NH,X/NH1) tend to have multiple saturated intervening absorbers with DR < 1.2. These results therefore indicate an additional contribution from the intervening system to the observed X-ray column density in some GRBs, although the contribution from the host galaxy alone cannot be excluded based on this study. © 2013. The American Astronomical Society. All rights reserved.

Cite

CITATION STYLE

APA

Wang, J. (2013). Evidence of contribution of intervening clouds to gamma-ray Burst’s X-ray column density. Astrophysical Journal, 776(2). https://doi.org/10.1088/0004-637X/776/2/96

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free