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Role of thermonuclear instabilities of recent models of nova-stars

Abstract

In this paper, a review models of nova-star explosion based on the original suggestion by Kraft and developed during about ten years (from 1967) is presented. The aim is to summarize the most salient results of those theoretical models and to point out the many aspects of the problems that are still unsettled. In particular, thermonuclear instabilities both in perfect and electron-degenerate gas are analyzed, 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:
AIX-14-766481; EDB-83-143515
Resource Relation:
Journal Name: Nuovo Cimento B; (Italy); Journal Volume: 65:2
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; NOVAE; NUCLEAR REACTIONS; ASTROPHYSICS; CNO CYCLE; ELECTRON GAS; LUMINOSITY; RADIATION PRESSURE; WHITE DWARF STARS; DWARF STARS; ERUPTIVE VARIABLE STARS; OPTICAL PROPERTIES; PHYSICAL PROPERTIES; STAR BURNING; STARS; VARIABLE STARS; 640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources
OSTI ID:
6120259
Country of Origin:
Italy
Language:
English
Other Identifying Numbers:
Journal ID: CODEN: NCIBA
Submitting Site:
HEDB
Size:
Pages: 345-403
Announcement Date:
Jun 01, 1983

Citation Formats

Secco, L. Role of thermonuclear instabilities of recent models of nova-stars. Italy: N. p., 1981. Web. doi:10.1007/BF02888825.
Secco, L. Role of thermonuclear instabilities of recent models of nova-stars. Italy. https://doi.org/10.1007/BF02888825
Secco, L. 1981. "Role of thermonuclear instabilities of recent models of nova-stars." Italy. https://doi.org/10.1007/BF02888825.
@misc{etde_6120259,
title = {Role of thermonuclear instabilities of recent models of nova-stars}
author = {Secco, L}
abstractNote = {In this paper, a review models of nova-star explosion based on the original suggestion by Kraft and developed during about ten years (from 1967) is presented. The aim is to summarize the most salient results of those theoretical models and to point out the many aspects of the problems that are still unsettled. In particular, thermonuclear instabilities both in perfect and electron-degenerate gas are analyzed, since they seem to be at the base of the nova explosion phenomena.}
doi = {10.1007/BF02888825}
journal = []
volume = {65:2}
journal type = {AC}
place = {Italy}
year = {1981}
month = {Oct}
}