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Simulations of RS Oph and the CSM in Type Ia Supernovae

Published online by Cambridge University Press:  29 January 2014

Richard A. Booth ,
Shazrene Mohamed  and
Philipp Podsiadlowski
Richard A. Booth
Affiliation:
Dept. of Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, United Kingdom email: richard.booth@astro.ox.ac.uk, podsi@astro.ox.ac.uk
Shazrene Mohamed
Affiliation:
South African Astronomical Observatory Observatory Road, Observatory, 7925, South Africa email: shazrene@saao.ac.za
Philipp Podsiadlowski
Affiliation:
Dept. of Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, United Kingdom email: richard.booth@astro.ox.ac.uk, podsi@astro.ox.ac.uk
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Abstract

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Smoothed particle hydrodynamics (SPH) models of the recurrent nova RS Ophiuchi are presented, along with simple models for circumstellar absorption lines. The evolution of the model sodium line is similar to the behaviour in some Type Ia SNe, e.g. SN2006X.

Keywords

hydrodynamicsbinaries: symbioticcircumstellar matterstars: individual (RS Oph)stars: novaecataclysmic variablessupernovae
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 382 - 383
Copyright
Copyright © International Astronomical Union 2014 

References

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