EDP Sciences Journals List
Advanced Search
Free access article

Issue A&A
Volume 451, Number 3, June I 2006
Page(s) 821 - 833
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20054085



A&A 451, 821-833 (2006)
DOI: 10.1051/0004-6361:20054085

Clustering of the optical-afterglow luminosities of long gamma-ray bursts

M. Nardini1, 2, G. Ghisellini1, G. Ghirlanda1, F. Tavecchio1, C. Firmani1, 3 and D. Lazzati4

1  Osservatorio Astronomico di Brera, via Bianchi 46, 23807 Merate, Italy
    e-mail: gabriele@merate.mi.astro.it
2  Univ. di Milano-Bicocca, P.za della Scienza 3, 20126 Milano, Italy
3  Instituto de Astronomía, UNAM, AP 70-264, 04510 México, DF, México
4  JILA, University of Colorado, Boulder, CO 80309-0440, USA

(Received 22 August 2005 / Accepted 16 January 2006)

Abstract
We studied the optical afterglows of the 24 pre-SWIFT gamma-ray bursts (GRBs) with both known spectroscopic redshift and published estimates of the optical extinction in the source frame. We found an unexpected clustering of the optical-afterglow luminosities measured 12 h (source frame time) after the trigger. For 21 out of 24 bursts, the distribution of the optical luminosities is narrower than the distribution of the X-ray luminosities, and even narrower than the distribution of the ratio between the monochromatic optical luminosities and the total isotropic, emitted prompt energy. Three bursts stand out from the distribution of the other sources, being underluminous by a factor ~15. We compare this result with another somewhat analogous result concerning the luminosity of the X-ray afterglows studied earlier. We constructed the optical to X-ray spectral energy distribution for all our GRBs. For all but a minority of them, the optical and the X-ray emissions are consistent with being produced by the same radiation process. We discuss our results in the framework of the "standard" external-shock synchrotron model. Finally, we consider the behavior of the first GRBs of known redshifts detected by SWIFT. We find that these SWIFT GRBs entirely confirm our findings.


Key words: gamma rays: bursts -- radiation mechanisms: non-thermal -- X-rays: general

SIMBAD Objects



© ESO 2006


What is OpenURL?

The OpenURL standard is a protocol for transmission of metadata describing the resource that you wish to access. An OpenURL link contains article metadata and directs it to the OpenURL server of your choice. The OpenURL server can provide access to the resource and also offer complementary services (specific search engine, export of references...). The OpenURL link can be generated by different means.
  • If your librarian has set up your subscription with an OpenURL resolver, OpenURL links appear automatically on the abstract pages.
  • You can define your own OpenURL resolver with your EDPS Account. In this case your choice will be given priority over that of your library.
  • You can use an add-on for your browser (Firefox or I.E.) to display OpenURL links on a page (see http://www.openly.com/openurlref/). You should disable this module if you wish to use the OpenURL server that you or your library have defined.