Figure 3 from Nebular Phase Observations of the Type Ib Supernova 2008D/X-ray Transient 080109: Side-viewed Bipolar Explosion

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Nebular Phase Observations of the Type Ib Supernova 2008D/X-ray Transient 080109: Side-viewed Bipolar Explosion

Authors: Masaomi Tanaka, Masayuki Yamanaka, Keiichi Maeda, Koji S. Kawabata, Takashi Hattori, Takeo Minezaki, Stefano Valenti, Massimo Della Valle, D. K. Sahu, G. C. Anupama, Nozomu Tominaga, Ken'ichi Nomoto, Paolo A. Mazzali, and Elena Pian

TANAKA et al. 2009 The Astrophysical Journal 700 1680.

Provider: AAS Journals

Caption: Figure 3.

Pseudobolometric light curve (black) of SN 2008D. The bolometric magnitudes are derived from UBVRIJHK magnitudes at early phases ( t _exp < 100 days; T. Minezaki 2009, in preparation) while they are estimated using the BC for SN 2002ap at late phases (Tomita et al. 2006). The solid lines in blue and green show the results of radiative transfer calculation by Tanaka et al. (2009). The gray line shows the total energy release from 0.07 M _☉ of ⁵⁶Ni.

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