NASA/IPAC EXTRAGALACTIC DATABASE
Date and Time of the Query: 2019-06-17 T22:14:56 PDT
Help | Comment | NED Home

For refcode 1989A&A...210..262H:
Retrieve 4 NED objects in this reference.
Please click here for ADS abstract

NED Abstract

Copyright by European Southern Observatory (ESO). Reproduced by permission
1989A&A...210..262H Theoretical models for the continuum and colors of SN 1979 C and SN 1980 K P.H. Hauschildt, G. Shaviv, and R. Wehrse Institut fur Theoretische Astrophysik, Im Neuenheimer Feld 561, D-6900 Heidelberg, Federal Republic of Germany Physics Department, TECHNION, IL-32000, Haifa, Israel Received March 22, accepted July 18, 1988 Summary. Models for the continuum energy distribution from supernovae of type II are constructed and compared with the recently observed SN 1979 C and SN 1980 K for the coasting phase of their evolution. Fairly good agreement with the observed energy distributions from the UV range down to the IR as well as with colors is found. Using the colors we demonstrate how the distance to the SN can be found. The advantage of this method relative to the classical Baade-Wesselink method is that it needs data only for a single time. Key words: supernovae - stellar atmospheres - distances
Retrieve 4 NED objects in this reference.
Please click here for ADS abstract

Back to NED Home