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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 4.

Nebular spectrum of SN 2008D (blue line) compared with that of SNe 1998bw (broad Ic; Patat et al. 2001), 2002ap (broad Ic; Mazzali et al. 2007), 2005kl (Ic; Maeda et al. 2008), and 2004gq (Ib; Maeda et al. 2008). The epochs are given as days since the explosion (days since the discovery are given for the two epochs marked with * as light curves are not available). The spectra are normalized to the peak flux of the [O i]λλ6300, 6364 line of SN 2008D. The spectra are shifted by 16, 12, 8, 4, and 0 from top to bottom for clarity.

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