Abstract
More than 40 supernovae have been observed at Asiago from the spectroscopic and/or photometric point of view (for a summary on the Asiago supernovae program, see the communication of Rosino, this conference). We have thus collected a fairly large and homogeneous set of data, from which we intend to deduce the main properties of both type I and II, and see whether these objects can be used as reliable distance indicators. In this communication the most recent results are presented in advance of publication (Barbon et al., 1973a, c). The most relevant data for nine supernovae are shown in Table I.
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References
Barbon, R., Ciatti, F., and Rosino, L.: 1973a, Mem. Soc. Astron. Ital. 44, 65.
Barbon, R., Ciatti, F., and Rosino, L.: 1973b, Astron. Astrophys. 25, 241.
Barbon, R., Ciatti, F., and Rosino, L.: 1973b, Astron. Astrophys. 25, 241.
Ciatti, F., Rosino, L., and Bertola, F.: 1971, Mem. Soc. Astron. Ital. 42, 163.
Goranskij, V. P.: 1973, Astron. Zirculiar,No. 723.
Sargent, W. L. W. and Searle, L.: 1973, IAU Circular, No. 2498.
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© 1974 D. Reidel Publishing Company, Dordrecht-Holland
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Barbon, R., Ciatti, F., Rosino, L. (1974). Recent Observations of Supernovae at Asiago. In: Cosmovici, C.B. (eds) Supernovae and Supernova Remnants. Astrophysics and Space Science Library, vol 45. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2166-1_13
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DOI: https://doi.org/10.1007/978-94-010-2166-1_13
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