Flat spectrum gamma ray burst afterglows

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1346

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DC Field	Value	Language
dc.contributor.author	Bhattacharya, D.	-
dc.date.accessioned	2006-06-12T06:43:40Z	-
dc.date.available	2006-06-12T06:43:40Z	-
dc.date.issued	2001-06	-
dc.identifier.citation	Bulletin of the Astronomical Society of India, 2001, Vol.29, p107-114	en
dc.identifier.issn	0304-9523	-
dc.identifier.uri	http://hdl.handle.net/2289/1346	-
dc.description.abstract	Temporal behaviour of GRB afterglow light curve is derived for the case where the electron energy distribution is relatively hard, with the power-law index p lying between 1.0 and 2.0. It is shown that the expected behaviour will be the same as that for p > 2.0 if the upper cutoff in the electron energy distribution evolves in direct proportion to the bulk Lorentz factor of the blast wave.	en
dc.format.extent	619131 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	The Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/cgi-bin/bib_query?2001BASI...29..107B	en
dc.rights	(2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.	en
dc.subject	Gamma Ray Burst	en
dc.subject	Afterglow	en
dc.subject	Radiation Mechanism	en
dc.subject	Theory	en
dc.title	Flat spectrum gamma ray burst afterglows	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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