Abstract
The growing interest on the issue of type I supernova homogeneity (see e.g. BRANCH et al. [1] and references therein) has suggested us to use all the spectroscopic material obtained at Asiago Observatory in the past years, through a fairly homogenous set of instrumentation, to give a contribution to the understanding of this important problem. Our first goal was to produce a temporal sequence of spectra defining a standard evolution for SNeI to be used as reference in search for peculiarities and, afterwards, to correlate these ones with other SN features such as the photometric parameters.
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References
Branch, D., Drucker, W., and Jeffery, D. J., 1988, Ap. J.(Letters), 330, L117.
Benetti, S. and Barbon, R. 1989, in preparation.
Pskovskii, Y. P. 1977, Soviet Astr., 21, 675.
Branch, D. 1981, Ap. J., 248, 1076.
Pskovskii, Y. P. 1984, Soviet Astr., 28, 658.
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Benetti, S., Barbon, R. (1991). Mean Evolution and Characteristics of Type I Supernova Spectra. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_70
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DOI: https://doi.org/10.1007/978-1-4612-2988-9_70
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