Preliminary spectral analysis of sn 1994i
Oct, 19957 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 279 (1996) 799
e-Print:
- astro-ph/9510070 [astro-ph]
View in:
Citations per year
Abstract: (arXiv)
We present optical spectra of the Type Ic supernova 1994I in M51 and preliminary non-LTE analysis of the spectra. Our models are not inconsistent with the explosions of C+O cores of massive stars. While we find no direct evidence for helium in the optical spectra, our models cannot rule out small amounts of helium. More than 0.1~\msol\ of helium seems unlikely.References(21)
Figures(0)