Hostname: page-component-8448b6f56d-dnltx Total loading time: 0 Render date: 2024-04-25T00:48:27.898Z Has data issue: false hasContentIssue false

Global parameters of Type Ia supernovae

Published online by Cambridge University Press:  01 August 2006

Bruno Leibundgut
Affiliation:
ESO, Karl-Schwarzschild-Strasse 3, D-85748 Garching, Germany email: bleibundgut@eso.org
Maximilian Stritzinger
Affiliation:
Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, DK-2100 Copenhagen Ø, Denmark email: max@dark-cosmology.dk
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.

Using simple physical assumptions we derived fundamental parameters including: the mass of synthesised 56Ni, the ejecta mass, and the explosion energy of Type Ia supernovae. The methods have been described in several recent publications and comparison with other methods shows general consistency.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2007

References

Arnett, W. D. 1982, ApJ, 253, 785CrossRefGoogle Scholar
Blinnikov, S., Röpke, F. K., Sorokina, E. I., Gieseler, M., Reinecke, M., Travaglio, C., Hillebrandt, W., & Stritzinger, M. 2006, A&A, 453, 229Google Scholar
Howell, A., et al. 2006, these proceedingsGoogle Scholar
Stritzinger, M., & Leibundgut, B. 2005, A&A, 431, 423Google Scholar
Stritzinger, M., Leibundgut, B., Walch, S., & Contardo, G. 2006a, A&A, 450, 241Google Scholar
Stritzinger, M., Mazzali, P., Sollerman, J., & Benetti, S. 2006b, A&A, 460, 793Google Scholar