dc.contributor.author |
Shanthi, K |
|
dc.contributor.author |
Bhat, C. L |
|
dc.date.accessioned |
2008-06-23T11:38:36Z |
|
dc.date.available |
2008-06-23T11:38:36Z |
|
dc.date.issued |
2002 |
|
dc.identifier.citation |
BASI, Vol. 30, No. 1, pp. 445 - 448 |
en |
dc.identifier.uri |
http://hdl.handle.net/2248/2490 |
|
dc.description.abstract |
A reclassification of the cosmic gamma-ray bursts has been done into two distinct classes on the basis of their brightness distributions. While one (majority) class is found to be compatible with a homogeneous and monoluminosity source population with simple cosmological effects folded into the brightness distribution function, the other, smaller population is not consistent with such a scenario and may need a consideration of source evolutionary effects. |
en |
dc.format.extent |
409530 bytes |
|
dc.format.mimetype |
application/pdf |
|
dc.language.iso |
en |
en |
dc.publisher |
Astronomical Society of India |
en |
dc.relation.uri |
http://adsabs.harvard.edu/abs/2002BASI...30..445S |
en |
dc.subject |
Cosmic Gamma Ray Bursts |
en |
dc.title |
Reclassification of gamma-ray bursts based on their brightness distributions |
en |
dc.type |
Article |
en |