J/ApJ/800/16             Swift-XRT long GRB durations             (Boer+, 2015)

Are ultra-long gamma-ray bursts different? Boer M., Gendre B., Stratta G. <Astrophys. J., 800, 16 (2015)> =2015ApJ...800...16B 2015ApJ...800...16B
ADC_Keywords: Gamma rays Keywords: gamma-ray burst: general Abstract: The discovery of a number of gamma-ray bursts (GRBs) with duration exceeding 1000s has opened the debate on whether these bursts form a new class of sources, the so-called ultra-long GRBs, or if they are rather the tail of the distribution of the standard long GRB duration. Using the long GRB sample detected by Swift, we investigate the statistical properties of long GRBs and compare them with the ultra-long burst properties. We compute the burst duration of long GRBs using the start epoch of the so-called "steep decay" phase detected with Swift/XRT. We discuss also the differences observed in their spectral properties. We find that ultra-long GRBs are statistically different from the standard long GRBs with typical burst duration less than 100-500s, for which a Wolf-Rayet star progenitor is usually invoked. Together with the presence of a thermal emission component we interpret this result as indication that the usual long GRB progenitor scenario cannot explain the extreme duration of ultra-long GRBs, their energetics, as well as the mass reservoir and size that can feed the central engine for such a long time. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 16 207 Our long GRB sample and the associated duration of the burst event in X-rays until the steep decay, taken from the XRT GRB catalog best fit parameters -------------------------------------------------------------------------------- See also: J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010) J/ApJ/701/824 : Afterglows of short & long-duration GRBs (Nysewander+, 2009) J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009) J/AJ/133/1027 : Positions for 179 Swift X-ray afterglows (Butler+, 2007) J/A+A/448/L9 : Position catalogue of Swift XRT afterglows (Moretti+, 2006) http://www.swift.ac.uk/xrt_live_cat : The Swift-XRT GRB online catalogue Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 7 A7 --- GRB Gamma Ray Burst identifier (YYMMDDA) 9- 16 F8.2 s TX [48/25400] Duration (TX) -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Greg Schwarz [AAS], Emmanuelle Perret [CDS] 25-Jun-2015
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