SwePub
Sök i LIBRIS databas

  Extended search

onr:"swepub:oai:DiVA.org:kth-15396"
 

Search: onr:"swepub:oai:DiVA.org:kth-15396" > A new definition of...

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

A new definition of the intermediate group of gamma-ray bursts

Horvath, I. (author)
Balazs, L. G. (author)
Bagoly, Z. (author)
show more...
Ryde, Felix (author)
Meszaros, A. (author)
show less...
2006-01-27
2006
English.
In: Astronomy and Astrophysics. - : EDP Sciences. - 0004-6361 .- 1432-0746. ; 447:1, s. 23-30
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • Gamma-ray bursts can be divided into three groups (short, intermediate, long) with respect to their durations. This classification is somewhat imprecise, since the subgroup of intermediate duration has an admixture of both short and long bursts. In this paper a physically more reasonable definition of the intermediate group is presented, using also the hardnesses of the bursts. It is shown again that the existence of the three groups is real, no further groups are needed. The intermediate group is the softest one. From this new definition it follows that 11% of all bursts belong to this group. An anticorrelation between the hardness and the duration is found for this subclass in contrast to the short and long groups. Despite this difference it is not clear yet whether this group represents a physically different phenomenon.

Keyword

gamma-rays : bursts
cosmology : miscellaneous
angular-distribution
anisotropy
identification
distributions
catalog

Publication and Content Type

ref (subject category)
art (subject category)

Find in a library

To the university's database

  • 1 of 1
  • Previous record
  • Next record
  •    To hitlist

Search outside SwePub

Kungliga biblioteket hanterar dina personuppgifter i enlighet med EU:s dataskyddsförordning (2018), GDPR. Läs mer om hur det funkar här.
Så här hanterar KB dina uppgifter vid användning av denna tjänst.

 
pil uppåt Close

Copy and save the link in order to return to this view