[AIT logo]

Institut für Astronomie und Astrophysik

Abteilung Astronomie

Sand 1, D-72076 Tübingen, Germany
[Uni logo]

Hinweis: Einige Seiten auf astro.uni-tuebingen.de können veraltet sein und werden nicht mehr aktualisiert.
Note: Some webpages at astro.uni-tuebingen.de may be outdated and will no longer be updated.


Preprint 06/06


Non-LTE modeling of supernova-fallback disks

K. Werner, T. Nagel, T. Rauch

Institut für Astronomie und Astrophysik, Universität Tübingen, Germany

To be published in: Astrophysics and Space Science

Abstract. We present a first detailed spectrum synthesis calculation of a supernova-fallback disk composed of iron. We assume a geometrically thin disk with a radial structure described by the classical alpha-disk model. The disk is represented by concentric rings radiating as plane-parallel slabs. The vertical structure and emission spectrum of each ring is computed in a fully self-consistent manner by solving the structure equations simultaneously with the radiation transfer equations under non-LTE conditions. We describe the properties of a specific disk model and discuss various effects on the emergent UV/optical spectrum. We find that strong iron-line blanketing causes broad absorption features over the whole spectral range. Limb darkening changes the spectral distribution up to a factor of four depending on the inclination angle. Consequently, such differences also occur between a blackbody spectrum and our model. The overall spectral shape is independent of the exact chemical composition as long as iron is the dominant species. A pure iron composition cannot be distinguished from silicon-burning ash. Non-LTE effects are small and restricted to few spectral features.
 

Preprint (979 kb PDF file including figures)
Astrophysics (astro-ph): astro-ph/0608529


[Home Page] [Preprints 2006] [Quick Reference] [Feedback]


Jürgen Barnstedt | Impressum
Last modified 30 Jan 2013
[Valid HTML 4.0!]