HOW FAR AWAY ARE GAMMA-RAY BURSTERS

Authors
Citation
B. Paczynski, HOW FAR AWAY ARE GAMMA-RAY BURSTERS, Publications of the Astronomical Society of the Pacific, 107(718), 1995, pp. 1167-1175
Citations number
68
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Publications of the Astronomical Society of the Pacific
ISSN journal
00046280 → ACNP
Volume
107
Issue
718
Year of publication
1995
Pages
1167 - 1175
Database
ISI
SICI code
0004-6280(1995)107:718<1167:HFAAGB>2.0.ZU;2-#
Abstract
The positions of over 1000 gamma-ray bursts detected with the BATSE ex periment on board the Compton Gamma Ray Observatory are uniformly and randomly distributed in the sky, with no significant concentration to the galactic plane or to the galactic center. The strong gamma-ray bur sts have an intensity distribution consistent with a number density in dependent of distance in Euclidean space. Weak gamma-ray bursts are re latively rare, indicating that either their number density is reduced at large distances or that the space in which they are distributed is non-Euclidean. In other words, we appear to be at the center of a sphe rical and bounded distribution of bursters. This is consistent with th e distribution of all objects that are known to be at cosmological dis tances (Like galaxies and quasars), but inconsistent with the distribu tion of any objects which are known to be in our galaxy (like stars an d globular clusters). If the bursters are at cosmological distances th en the weakest bursts should be redshifted, i.e., on average their dur ations should be longer and their spectra should be softer than the co rresponding quantities for the strong bursts. There is some evidence f or both effects in the BATSE data. At this time the cosmological dista nce scale is strongly favored over the galactic one, but is not proven . A definite proof (or disproof) could be provided with the results of a search for very weak bursts in the Andromeda galaxy (M31) with an i nstrument similar to 10 times more sensitive than BATSE. If the burste rs are indeed at cosmological distances then they are the most luminou s sources of electromagnetic radiation known in the Universe. At this time we have no clue as to their nature, even though well over a hundr ed suggestions have been published in the scientific journals. An expe riment providing similar to 1 arcsecond positions would greatly improv e the likelihood that counterparts of gamma-ray bursters are finally f ound. A new interplanetary network would offer the best opportunity.