Nalazite se na CroRIS probnoj okolini. Ovdje evidentirani podaci neće biti pohranjeni u Informacijskom sustavu znanosti RH. Ako je ovo greška, CroRIS produkcijskoj okolini moguće je pristupi putem poveznice www.croris.hr
izvor podataka: crosbi

Energetics-spectral correlations versus the BATSE gamma-ray bursts population (CROSBI ID 260423)

Prilog u časopisu | izvorni znanstveni rad | međunarodna recenzija

Bošnjak, Željka ; Celotti, A. ; Longo, F. ; Barbiellini, G. Energetics-spectral correlations versus the BATSE gamma-ray bursts population // Monthly notices of the Royal Astronomical Society, 384 (2008), 2; 599-604. doi: 10.1111/j.1365-2966.2007.12672.x

Podaci o odgovornosti

Bošnjak, Željka ; Celotti, A. ; Longo, F. ; Barbiellini, G.

engleski

Energetics-spectral correlations versus the BATSE gamma-ray bursts population

The proposed correlations between the energetics of gamma-ray bursts (GRBs) and their spectral properties, namely the peak energy of their prompt emission, can broadly account for the observed fluence distribution of all `bright' BATSE GRBs, under the hypothesis that the GRB rate is proportional to the star formation rate and that the observed distribution in peak energy is independent of redshift. The correlations can also be broadly consistent with the properties of the whole BATSE long GRB population for a peak energy distribution smoothly extending towards lower energies, and in agreement with the properties of a sample at `intermediate' fluences and with the luminosity functions inferred from the GRB number counts. We discuss the constraints that this analysis imposes on the shape of such peak energy distribution, the opening angle distribution and the tightness of the proposed correlations.

gamma-rays: bursts

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

nije evidentirano

Podaci o izdanju

384 (2)

2008.

599-604

objavljeno

0035-8711

1365-2966

10.1111/j.1365-2966.2007.12672.x

Povezanost rada

Fizika

Poveznice
Indeksiranost