Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-23T10:33:38.776Z Has data issue: false hasContentIssue false
  • English
  • Français

White Dwarf Model Atmospheres: Synthetic Spectra for Supersoft Sources

Published online by Cambridge University Press:  17 January 2013

Thomas Rauch
Thomas Rauch*
Affiliation:
Institute for Astronomy and Astrophysics, Kepler Center for Astro and Particle Physics, Eberhard Karls University, Sand 1, 72076 Tübingen, Germany email: rauch@astro.uni-tuebingen.de
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The Tübingen NLTE Model-Atmosphere Package (TMAP) calculates fully metal-line blanketed white dwarf model atmospheres and spectral energy distributions (SEDs) at a high level of sophistication. Such SEDs are easily accessible via the German Astrophysical Virtual Observatory (GAVO) service TheoSSA. We discuss applications of TMAP models to (pre) white dwarfs during the hottest stages of their stellar evolution, e.g. in the parameter range of novae and supersoft sources.

Keywords

astronomical data bases: miscellaneous — stars: abundancesAGB and post-AGBatmospheresearly-typeindividual (V 4743 Sgr, V 1974 Cyg)novaecataclysmic variableswindsoutflows — binaries: close — X-rays: binariesbursts
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Issue S281: Binary Paths to Type Ia Supernovae Explosions , July 2011 , pp. 60 - 63
Copyright
Copyright © International Astronomical Union 2013

References

González-Riestra, R. & Krautter, J. 1998, in: Wamsteker, W., González-Riestra, R. (eds.), Ultraviolet Astrophysics Beyond the IUE Final Archive, ESA SP, 413, 367Google Scholar
Hauschildt, P. H. & Baron, E. 1999, J. of Computational and Applied Mathematics, 109, 41Google Scholar
Ness, J.-U., Starrfield, S., Burwitz, V., et al. 2003, ApJ 594 L 127Google Scholar
Ness, J.-U. 2010, AN, 331, 179Google Scholar
Rauch, T. 2011, in: The X-ray Universe 2011, available online at: http://xmm.esac.esa.int/external/xmm_science/workshops/2011symposium/, 61Google Scholar
Rauch, T., Orio, M., Gonzáles-Riestra, R., Nelson, T., et al. 2010, ApJ, 717, 363CrossRefGoogle Scholar
Rauch, T. & Deetjen, J. L. 2003, in: Hubeny, I., Mihalas, D., Werner, K. (eds.), Stellar Atmosphere Modeling, The ASP Conference Series (San Francisco: ASP), 288, 103Google Scholar
Rauch, T. & Werner, K. 2010, AN, 331, 146Google Scholar
Rauch, T., Ringat, E., & Werner, K. 2011, Universal Academy Press, in press, arXiv:1011.3628Google Scholar
van Rossum, D. R. & Ness, J.-U. 2010, AN, 331, 175Google Scholar
Werner, K., Dreizler, S., Deetjen, J. L., Nagel, T., Rauch, T., & Schuh, S. L. 2003, in: Hubeny, I., Mihalas, D., Werner, K. (eds.), Stellar Atmosphere Modeling, The ASP Conference Series (San Francisco: ASP), 288, 31Google Scholar