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Journal article

The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant

Abstract:: We present a model for the type Ia supernova remnant (SNR) of SN 1604, also known as Kepler's SNR. We find that its main features can be explained by a progenitor model of a symbiotic binary consisting of a white dwarf and an AGB donor star with an initial mass of 4-5 M ⊙. The slow, nitrogen-rich wind emanating from the donor star has partially been accreted by the white dwarf, but has also created a circumstellar bubble. On the basis of observational evidence, we assume that the system moves...
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Publication status:: Published

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APA Style

Chiotellis, A., Schure, K., & Vink, J. (2012). The imprint of a symbiotic binary progenitor on the properties of Kepler's supernova remnant. ASTRONOMY and ASTROPHYSICS, 537, A139–A139.

MLA Style

Chiotellis, A., et al. “The Imprint of a Symbiotic Binary Progenitor on the Properties of Kepler's Supernova Remnant.” ASTRONOMY and ASTROPHYSICS, vol. 537, 2012, pp. A139–A139.

Chicago Style

Chiotellis, A, K Schure, and J Vink. 2012. “The Imprint of a Symbiotic Binary Progenitor on the Properties of Kepler's Supernova Remnant.” ASTRONOMY and ASTROPHYSICS 537: A139–A139.
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Publisher copy:: 10.1051/0004-6361/201014754

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+ Chiotellis, A More by this author

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+ Schure, K More by this author

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+ Vink, J More by this author

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Bibliographic Details

Journal:: ASTRONOMY and ASTROPHYSICS
Volume:: 537
Pages:: A139-A139
Publication date:: 2012-01-01
DOI:: 10.1051/0004-6361/201014754
EISSN:: 1432-0746
ISSN:: 0004-6361

Item Description

Language:: English
Keywords:: supernovae: individual: SN1604

binaries: symbiotic

hydrodynamics

ISM: supernova remnants
Pubs id:: pubs:313538
UUID:: uuid:3a70ba7e-3db1-4889-84e9-1b165f47d09c
Local pid:: pubs:313538
Source identifiers:: 313538
Deposit date:: 2012-12-19

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Copyright date:: 2012

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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