Hostname: page-component-848d4c4894-ndmmz Total loading time: 0 Render date: 2024-05-01T16:55:41.871Z Has data issue: false hasContentIssue false

The common-envelope wind model for type Ia supernovae

Published online by Cambridge University Press:  30 December 2019

Xiangcun Meng
Affiliation:
Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, PR China email: xiangcunmeng@ynao.ac.cn
Philipp. Podsiadlowski
Affiliation:
Department of Astronomy, Oxford University, Oxford OX1 3RH, UK
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.

We have developed a new version of the SD model for type Ia supernovae (SNe Ia) in which a common envelope (CE) is assumed to form if the mass-transfer rate between a carbon/oxygen white dwarf (CO WD) and its companion exceeds a critical accretion rate. Based on this model, we found that both SN 2002cx-like and SN Ia-CSM objects may share a similar origin, i.e. these peculiar objects may originate from the explosion of hybrid carbon/oxygen/neon white dwarfs (CONe WDs) in SD systems, where SNe Ia-CSM explode in systems with a massive CE of ∼1 M, while SN 2002cx-like events correspond to events without a massive CE.

Type
Contributed Papers
Copyright
© International Astronomical Union 2019 

References

Hachisu, I., Kato, M., Nomoto, K. 1996, ApJ, 470, L97 CrossRefGoogle Scholar
Maoz, D., Mannucci, F., Nelemans, G. 2014, ARAA, 52, 107 CrossRefGoogle Scholar
Meng, X. & Podsiadlowski, Ph. 2017, MNRAS, 469, 4763 CrossRefGoogle Scholar
Meng, X. & Podsiadlowski, Ph. 2018, ApJ, 861,127 CrossRefGoogle Scholar
Perlmutter, S., Aldering, G., Goldhaber, G., et al. 1999, ApJ, 517, 565 CrossRefGoogle Scholar
Riess, A., Filippenko, A. V., Challis, P., et al. 1998, AJ, 116, 1009 CrossRefGoogle Scholar
Rodney, S. A. et al. 2015, AJ, 150, 156 CrossRefGoogle Scholar