Titre du document

On the Nature of Strong Radio Sources

Lien vers le document
Nom du Corpus

AstroConcepts

Auteur(s)
  • F. Hoyle
  • William A. Fowler
Résumé

The events leading to strong radio emission are taken to originate in the nucleus of a galaxy. But instead of outbursts from a large number of stars of ordinary mass, the possibility is considered of the existence at the very centre of a stellar-type object of large mass. The evolution of such an object is considered. After hydrogen burning and helium burning, neutrino emission leads to a collapse that initiates an explosive burning of oxygen. The star then disintegrates at a speed of 5000 km sec?1 or more. Our preference, however, is not for this final outburst as the process leading to radio emission. Rather do we prefer, analogously to the case of the solar system, the process of formation in which angular momentum is transferred from the central star to a surrounding disk of gas.

Langue(s) du document
Indéterminé
Année de publication
1962
Revue

Monthly Notices of the Royal Astronomical Society

Éditeur
OUP
Type de publication
journal
Type de document
research-article
Présence de XML structuré
Non
Version de PDF
1.4
Score de qualité du texte
3.633
Nom du concept
  • CNO cycles
  • Seyfert galaxies
Catégories Science-Metrix
  • 1 - natural sciences ; 2 - physics & astronomy ; 3 - astronomy & astrophysics
Catégories Inist
  • 1 - sciences appliquees, technologies et medecines ; 2 - sciences exactes et technologie ; 3 - terre, ocean, espace ; 4 - geophysique externe
Catégories Scopus
  • 1 - Physical Sciences ; 2 - Earth and Planetary Sciences ; 3 - Space and Planetary Science
  • 1 - Physical Sciences ; 2 - Physics and Astronomy ; 3 - Astronomy and Astrophysics
Catégories WoS
  • 1 - science ; 2 - astronomy & astrophysics
Identifiant ISTEX
F7DFA70550027BB4428BC30BC106A0D8E60FD3A7
ark:/67375/HXZ-2SQZWMK9-4
Powered by Lodex 9.4.5