Journal Article

Observational constraints on the external shock prior emission hypothesis of gamma-ray bursts

Tesla Birnbaum, Bing Zhang, Bin-Bin Zhang and En-Wei Liang

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 422, issue 1, pages 393-400
Published in print May 2012 | ISSN: 0035-8711
Published online April 2012 | e-ISSN: 1365-2966 | DOI:
Observational constraints on the external shock prior emission hypothesis of gamma-ray bursts

More Like This

Show all results sharing this subject:

  • Astronomy and Astrophysics


Show Summary Details


An intriguing hypothesis that there exists a decaying X-ray emission component before the gamma-ray burst (GRB) trigger has been suggested in order to explain the shallow decay phase of the X-ray afterglow detected in many Swift GRBs. If this ‘prior emission’ is from an external shock, one would expect a corresponding optical emission component during the GRB prompt emission phase. In this paper we apply the available prompt optical emission data (both detections and upper limits) to constrain such a scenario. We fit the shallow and normal decay segments of the X-ray Telescope light curves in our sample with a TΔ-shifted single power law, and extrapolate the X-ray flux back to the time of the early optical observations. We then use the synchrotron spectrum predicted by the standard external shock model to extrapolate from the X-ray flux to the optical band, and obtain the possible range of the predicted optical flux. Finally, we compare the predictions with the observations. In the cases where later optical data are available, we also compare the shapes of the optical light curves to the predicted optical light curves from the external shock prior emission model. We find that for a good fraction of GRBs (four out of eight; up to 2006 December), the available data already impose severe constraints on the hypothesis. In particular, the expected optical flux from the external shock prior emission model is higher than what the data allow. We conclude that if the shallow-decay X-ray component were from a prior emission component, it would have to be of an internal origin with optical flux suppressed.

Keywords: radiation mechanisms: non-thermal; shock waves; gamma-ray burst: general

Journal Article.  5982 words.  Illustrated.

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.