Fig. 3 from The Unique Type Ib Supernova 2005bf: A WN Star Explosion Model for Peculiar Light Curves and Spectra

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The Unique Type Ib Supernova 2005bf: A WN Star Explosion Model for Peculiar Light Curves and Spectra

Authors: N. Tominaga, M. Tanaka, K. Nomoto, P. A. Mazzali, J. Deng, K. Maeda, H. Umeda, M. Modjaz, M. Hicken, P. Challis, R. P. Kirshner, W. M. Wood-Vasey, C. H. Blake, J. S. Bloom, M. F. Skrutskie, A. Szentgyorgyi, E. E. Falco, N. Inada, T. Minezaki, Y. Yoshii, K. Kawabata, M. Iye, G. C. Anupama, D. K. Sahu, and T. P. Prabhu

Tominaga et al. 2005 The Astrophysical Journal Letters 633 L97.

Caption: Fig. 3.

Time evolution of the He line velocity derived from the absorption minimum of He I λ5876 (M. Modjaz et al. 2005, in preparation).