Sie befinden Sich nicht im Netzwerk der Universität Paderborn. Der Zugriff auf elektronische Ressourcen ist gegebenenfalls nur via VPN oder Shibboleth (DFN-AAI) möglich. mehr Informationen...
Ergebnis 2 von 11
The Astrophysical journal, 2012-10, Vol.757 (2), p.1-14
2012
Volltextzugriff (PDF)

Details

Autor(en) / Beteiligte
Titel
SUPERLUMINOUS LIGHT CURVES FROM SUPERNOVAE EXPLODING IN A DENSE WIND
Ist Teil von
  • The Astrophysical journal, 2012-10, Vol.757 (2), p.1-14
Ort / Verlag
United States
Erscheinungsjahr
2012
Quelle
EZB Electronic Journals Library
Beschreibungen/Notizen
  • Observations from the last decade have indicated the existence of a general class of superluminous supernovae (SLSNe), in which the peak luminosity exceeds 10 super(44) erg s super(-l). Here we focus on a subclass of these events, where the light curve is also tens of days wide, so the total radiated energy is of order 10 super(51) erg. We examine the scenario where the radiated luminosity is due to efficient conversion of kinetic energy of the ejected stellar envelope into radiation by interaction with an optically thick, pre-existing circumstellar material, presumably the product of a steady wind from the progenitor. We base the analysis on analytical derivations of various limits, and on a simple, numerically solved, hydrodynamic diffusion model, which allows us to explore the regime of interest, which does not correspond to the analytical limits. In our results, we identify the qualitative behavior of the observable light curves, and relate them to the parameters of the wind.

Weiterführende Literatur

Empfehlungen zum selben Thema automatisch vorgeschlagen von bX