Colors of the Optical Afterglow of GRB030329/SN 2003dh

Details Colors of the Optical Afterglow of GRB030329/SN 2003dh Colors of the Optical Afterglow of GRB030329/SN 2003dh

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aipc..727..339s&link_type=abstract

GAMMA-RAY BURSTS: 30 YEARS OF DISCOVERY: Gamma-Ray Burst Symposium. AIP Conference Proceedings, Volume 727, pp. 339-340 (2004).

Other

Gamma-Ray Sources, Gamma-Ray Bursts, Supernovae, Magnitudes And Colors, Luminosities

Scientific paper

We show that the color indices (B - V)0, (V - R)0, (R - I)0 of the optical afterglow of GRB030329 were consistent with those of the other OAs during t - T0 < 10 days. This suggests that the synchrotron component was initially dominant in the spectrum. Large color variations emerge only for t - T0 > 20 days and suggest a rapid spectral evolution of the underlying supernova SN 2003dh.

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