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2006CBET..368....3G - Central Bureau Electronic Telegrams, 368, 3 (2006/January-0)
Supernovae 2006F and 2006G.
GREEN D.W.E.
Abstract (from CDS):
SN 2006G is a type-II supernova with a strong H_alpha P-Cyg feature and some metallic lines. Weak H_beta is detected in absorption, indicating an expansion velocity of 10000 km/s, if one assumes the NED recession velocity of 5018 km/s for the host galaxy (from Huchra et al. 1999, Ap.J. Suppl. 121, 287). The presence of Fe II 516.9-nm and the high expansion velocity derived from H_beta suggest that the supernova is 2-3 weeks old.
Abstract Copyright: ∼
Journal keyword(s):
Simbad objects: 2
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