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Role of thermonuclear instability in recent models of nova stars

Abstract

In this paper we review models of nova-star explosion based on the original suggestion by Kraft and developed during about ten years (from 1967). We aim at summarizing here the most salient results of those theoretical models and to point out the many aspects of the problems that are still unsettled. In particular, we analyse thermonuclear instabilities both in perfect and electron-degenerate gas, since they seem to be at the base of the nova explosion phenomena.
Authors:
Secco, L [1] 
  1. Padua Univ. (Italy). Ist. di Astronomia
Publication Date:
Oct 11, 1981
Product Type:
Journal Article
Reference Number:
EDB-83-052968
Resource Relation:
Journal Name: Nuovo Cimento B; (Italy); Journal Volume: 65:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; NOVAE; THERMONUCLEAR EXPLOSIONS; COMPARATIVE EVALUATIONS; ELECTRON GAS; INSTABILITY; STAR MODELS; ERUPTIVE VARIABLE STARS; EXPLOSIONS; MATHEMATICAL MODELS; NUCLEAR EXPLOSIONS; STARS; VARIABLE STARS; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
6488385
Country of Origin:
Italy
Language:
Italian
Other Identifying Numbers:
Journal ID: CODEN: NCIBA
Submitting Site:
HEDB
Size:
Pages: 345-403
Announcement Date:

Citation Formats

Secco, L. Role of thermonuclear instability in recent models of nova stars. Italy: N. p., 1981. Web. doi:10.1007/BF02888825.
Secco, L. Role of thermonuclear instability in recent models of nova stars. Italy. doi:10.1007/BF02888825.
Secco, L. 1981. "Role of thermonuclear instability in recent models of nova stars." Italy. doi:10.1007/BF02888825. https://www.osti.gov/servlets/purl/10.1007/BF02888825.
@misc{etde_6488385,
title = {Role of thermonuclear instability in recent models of nova stars}
author = {Secco, L}
abstractNote = {In this paper we review models of nova-star explosion based on the original suggestion by Kraft and developed during about ten years (from 1967). We aim at summarizing here the most salient results of those theoretical models and to point out the many aspects of the problems that are still unsettled. In particular, we analyse thermonuclear instabilities both in perfect and electron-degenerate gas, since they seem to be at the base of the nova explosion phenomena.}
doi = {10.1007/BF02888825}
journal = {Nuovo Cimento B; (Italy)}
volume = {65:2}
journal type = {AC}
place = {Italy}
year = {1981}
month = {Oct}
}