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Nature of type 1 supernovae
| Content Provider | NASA Technical Reports Server (NTRS) |
|---|---|
| Author | Shklovskiy, I. S. |
| Copyright Year | 1980 |
| Description | The nature of type 1 supernovae (SN 1) is discussed through a comparison of observational evidence and theoretical perspectives relating to both type 1 and 2 supernovae. In particular two hypotheses relating to SN 1 phenomenon are examined: the first proposing that SN 1 are components of binary systems in which, at a comparatively late stage of evolution, overflow of the mass occurs; the second considers pre-SN 1 to be recently evolved stars with a mass greater than 1.4 solar mass (white dwarfs). In addition, an explanation of the reduced frequency of flares of SN 1 in spiral galaxies as related to that in elliptical galaxies is presented. |
| File Size | 2861942 |
| Page Count | 38 |
| File Format | |
| Alternate Webpage(s) | http://archive.org/details/NASA_NTRS_Archive_19800019778 |
| Archival Resource Key | ark:/13960/t75t8fm5f |
| Language | English |
| Publisher Date | 1980-06-01 |
| Access Restriction | Open |
| Subject Keyword | Astrophysics Stellar Envelopes Supernova Remnants Neutron Stars White Dwarf Stars Elliptical Galaxies Supernovae Stellar Mass Binary Stars Stellar Evolution Planetary Nebulae Spiral Galaxies Ntrs Nasa Technical Reports Server (ntrs) Nasa Technical Reports Server Aerodynamics Aircraft Aerospace Engineering Aerospace Aeronautic Space Science |
| Content Type | Text |
| Resource Type | Technical Report |
