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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. Lazzati41 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
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