Published 1988
| Version v1
Book
The circumstellar structure around supernovae
Creators
- 1. Lund Observatory (Sweden)
- 2. Stockholm Observatory (Sweden)
Description
The time dependent ionization and temperature structure of the circumstellar medium around supernovae has been calculated, in order to interpret recent supernova radio observations. For a stellar wind origin of the circumstellar medium, the authors relate the time of radio turn-on to the progenitor mass loss rate. They also show that large column densities for the UV resonance lines are expected. The results are applied to SN 1979c, SN 1980K and SN 1987A
Additional details
Publishing Information
- Publisher
- Cambridge University Press.
- Imprint Place
- New York, NY (USA)
- ISBN
- 0-521-35062-X
- Imprint Title
- Supernova remnants and the interstellar medium
- Imprint Pagination
- 535 p.
- Journal Page Range
- p. 15-18.
Conference
- Title
- 101. International Astronomics Union colloquium on interaction of supernova remnants with the interstellar medium.
- Dates
- 8-12 Jun 1987.
- Place
- Penticton (Canada).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 22001192
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- INTERSTELLAR SPACE; IONIZATION; MASS; STELLAR WINDS; SUPERNOVAE; TEMPERATURE GRADIENTS; TIME DEPENDENCE
- Descriptors DEC
- BINARY STARS; ERUPTIVE VARIABLE STARS; SPACE; STARS; STELLAR ACTIVITY; VARIABLE STARS
Optional Information
- Secondary number(s)
- CONF-8706201--.