Echo Emission from Dust Scattering and X-Ray Afterglows of Gamma-Ray Bursts

dc.contributor.authorShao, L.
dc.contributor.authorDai, Z. G.
dc.contributor.authorMirabal, Nestor
dc.date.accessioned2020-09-04T18:23:37Z
dc.date.available2020-09-04T18:23:37Z
dc.date.issued2007-11-23
dc.description.abstractWe investigate the effect of X-ray echo emission in gamma-ray bursts (GRBs). We find that the echo emission can provide an alternative way of understanding X-ray shallow decays and jet breaks. In particular, a shallow decay followed by a "normal" decay and a further rapid decay of X-ray afterglows can together be explained as being due to the echo from prompt X-ray emission scattered by dust grains in a massive wind bubble around a GRB progenitor. We also introduce an extra temporal break in the X-ray echo emission. By fitting the afterglow light curves, we can measure the locations of the massive wind bubbles, which will bring us closer to finding the mass-loss rate, wind velocity, and age of the progenitors prior to the GRB explosions.en
dc.description.sponsorshipThanks to the Swift satellite (Gehrels et al. 2004), our interpretation of GRBs has become more complex. The feature of a shallow decay followed by a “normal” decay and a further rapid decay of X-ray afterglows appears to be canonical (Zhang et al. 2006; Nousek et al.2006). Coincidentally, we find that this feature can be naturally reproduced by the echo emission.en
dc.description.urihttps://iopscience.iop.org/article/10.1086/527047en
dc.format.extent25 pagesen
dc.genrejournal articles preprintsen
dc.identifierdoi:10.13016/m2naq5-pkpy
dc.identifier.citationL. Shao, Z. G. Dai and N. Mirabal, Echo Emission from Dust Scattering and X-Ray Afterglows of Gamma-Ray Bursts, ApJ 675 507 (2008), doi: https://doi.org/10.1086/527047en
dc.identifier.urihttps://doi.org/10.1086/527047
dc.identifier.urihttp://hdl.handle.net/11603/19596
dc.language.isoenen
dc.publisherIOPen
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Physics Department Collection
dc.relation.ispartofUMBC Joint Center for Earth Systems Technology (JCET)
dc.relation.ispartofUMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
dc.rightsThis item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author.
dc.rights© 2008. The American Astronomical Society. All rights reserved.
dc.titleEcho Emission from Dust Scattering and X-Ray Afterglows of Gamma-Ray Burstsen
dc.typeTexten

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