Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aipc..662..338s&link_type=abstract
GAMMA-RAY BURST AND AFTERGLOW ASTRONOMY 2001: A Workshop Celebrating the First Year of the HETE Mission. AIP Conference Proceed
Astronomy and Astrophysics
Astronomy
Gamma-Ray Sources, Gamma-Ray Bursts, Photography And Photometry
Scientific paper
The study of the color indices and luminosities of 17 optical afterglows (OAs) of GRBs, including the most recent one, GRB010222, showed that the color variations during the decline of OAs are quite small during t - T0 < 10 days and allow a comparison among them, even for the less densely sampled OAs. The colors in the observer frame concentrate at (V - R)0 = 0.40+/-0.13, (R - I)0 = 0.46+/-0.18, (B - V)0 = 0.47+/-0.17, except for GRB000131 and GRB980425. However, large scatter is observed in (U - B)0. The color evolution of the OAs is negligible although their brightness declines by several magnitudes during t - T0 < 10 days. Such a strong concentration of the color indices also suggests that the intrinsic reddening (inside their host galaxies) must be quite similar and relatively small for all these events. The absolute brightness of OAs in the observer frame lies within MR
Hudec Rene
Masetti Nicola
Pizzichini Graziella
Simon Veronica
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