Energies of X-ray plateaus and flares in GRBs Virtual Observatory Resource

Authors
  1. Yi S.-X.
  2. Du M.
  3. Liu T.
  4. Published by
    CDS
Abstract

Distinct X-ray plateau and flare phases have been observed in the afterglows of gamma-ray bursts (GRBs), and most of them should be related to central engine activities. In this paper, we collect 174 GRBs with X-ray plateau phases and 106 GRBs with X-ray flares. There are 51 GRBs that overlap in the two selected samples. We analyze the distributions of the proportions of the plateau energy Eplateau and the flare energy E_flare_ relative to the isotropic prompt emission energy E_{gamma},iso_. The results indicate that they well meet the Gaussian distributions and the medians of the logarithmic ratios are ~-0.96 and -1.39 in the two cases. Moreover, strong positive correlations between E_plateau_ (or E_flare_) and E_{gamma},iso_ with slopes of ~0.95 (or ~0.80) are presented. For the overlapping sample, the slope is ~0.80. We argue that most of X-ray plateaus and flares might have the same physical origin but appear with different features because of the different circumstances and radiation mechanisms. We also test the applicabilities of two models, i.e., black holes surrounded by fractured hyperaccretion disks and millisecond magnetars, on the origins of X-ray plateaus and flares.

Keywords
  1. gamma-ray-astronomy
  2. gamma-ray-bursts
  3. redshifted
  4. x-ray-sources
  5. spectral-energy-distribution
Bibliographic source Bibcode
2022ApJ...924...69Y
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/924/69
IVOA Identifier IVOID
ivo://CDS.VizieR/J/ApJ/924/69
Document Object Identifer DOI
doi:10.26093/cds/vizier.19240069

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History

2023-08-28T10:29:24Z
Resource record created
2023-08-28T10:29:24Z
Created
2023-11-03T13:25:45Z
Updated

Contact

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