Testing for synchrotron self-absorption in GRB 970111

Citation
A. Crider et Ep. Liang, Testing for synchrotron self-absorption in GRB 970111, ASTR AST SS, 138(3), 1999, pp. 405-406
Citations number
13
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
ISSN journal
03650138 → ACNP
Volume
138
Issue
3
Year of publication
1999
Pages
405 - 406
Database
ISI
SICI code
0365-0138(199909)138:3<405:TFSSIG>2.0.ZU;2-5
Abstract
The time-resolved spectra of several gamma-ray bursts have shown that near the beginning of the burst, some absorption mechanism makes the spectra inc onsistent with the simple optically-thin synchrotron shock model. We fit GR B 970111, which shows strong evidence for such absorption, with a synchrotr on shock spectra suffering self-absorption. The synchrotron self-absorption shape does fit the BATSE time-evolving spectra, although it may be inconsi stent with BeppoSAX WFC data. If the turnover just below the spectral break is due to synchrotron self-absorption, a magnetic field strength of 4 10(7 ) G is required.