A new survey of X-ray flares

J. Mao*, G. Chincarini, C. Guidorzi, R. Margutti, M. G. Bernardini, F. Pasotti

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

One of the most interesting discoveries of the Swift mission is the wide variety of X-ray behaviors observed in the early GRB afterglows. We selected a large sample of bright X-ray flares observed by XRT up to March 2008. The Norris et al. (2005) profile was adopted to characterize the morphological and timing properties of the flares in different energy bands, such as the peak, rise and decay times, the width and the asymmetry of each flare. These parameters were used to estimate other properties in a homogeneous way, such as the temporal lag between the same pulse seen at different energy bands, or the width of the flare as a function of energy, thus allowing us to derive important clues on the underlying physical mechanism and the connections with the central engine.

Original languageEnglish (US)
Title of host publication2008 Nanjing Gamma-Ray Burst Conference
Pages31-34
Number of pages4
DOIs
StatePublished - Dec 1 2008
Event2008 Nanjing Gamma-Ray Burst Conference - Nanjing, China
Duration: Jun 23 2008Jun 27 2008

Publication series

NameAIP Conference Proceedings
Volume1065
ISSN (Print)0094-243X
ISSN (Electronic)1551-7616

Other

Other2008 Nanjing Gamma-Ray Burst Conference
CountryChina
CityNanjing
Period6/23/086/27/08

Keywords

  • γ-ray burst
  • γ-ray sources

ASJC Scopus subject areas

  • Physics and Astronomy(all)

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