Published 1986
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Neutron star formation in theoretical supernovae. Low mass stars and white dwarfs
Description
The presupernova evolution of stars that form semi-degenerate or strongly degenerate O + Ne + Mg cores is discussed. For the 10 to 13 Msub solar stars, behavior of off-center neon flashes is crucial. The 8 to 10 m/sub solar stars do not ignite neon and eventually collapse due to electron captures. Properties of supernova explosions and neutron stars expected from these low mass progenitors are compared with the Crab nebula. The conditions for which neutron stars form from accretion-induced collapse of white dwarfs in clsoe binary systems is also examined
Availability note (English)
MF available from INIS under the Report Number; Available from NTIS, PC A02/MF A01; 1 as DE86016168.Files
18096982.pdf
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Additional details
Publishing Information
- Imprint Pagination
- 24 p.
- Report number
- BNL--38555
Conference
- Title
- Conference on the origin and evolution of neutron stars.
- Dates
- 26-30 May 1986.
- Place
- Nanjing (China).
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 18096982
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCRETION DISKS; MAGNESIUM; NEON; NEUTRON STARS; OXYGEN; SUPERNOVAE; SYNTHESIS; WHITE DWARF STARS
- Descriptors DEC
- ALKALINE EARTH METALS; BINARY STARS; DWARF STARS; ELEMENTS; ERUPTIVE VARIABLE STARS; METALS; NONMETALS; RARE GASES; STARS; VARIABLE STARS
Optional Information
- Notes
- Portions of this document are illegible in microfiche products.
- Secondary number(s)
- CONF-8605190--1.