(Q56061239)

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The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in type Ia supernovae

scientific article published in Astronomy and Astrophysics

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The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in type Ia supernovae (English)

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F. K. Röpke

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1

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W. Hillebrandt

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2

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English

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publication date

14 May 2004

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Astronomy and Astrophysics

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420

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1

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page(s)

1–4

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cites work

A possible model of supernovae: Detonation of12C

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Crossref

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https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

Type I supernovae. I - Analytic solutions for the early part of the light curve

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https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

Thermonuclear supernovae: simulations of the deflagration stage and their implications

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https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

Type Ia Supernova Explosion Models

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https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

Fronts propagating with curvature-dependent speed: Algorithms based on Hamilton-Jacobi formulations

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https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

The absolute magnitudes of Type IA supernovae

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reference URL

https://api.crossref.org/works/10.1051%2F0004-6361%3A20040135

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21 January 2018

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10.1051/0004-6361:20040135

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ResearchGate publication ID

1797895

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(Q56061239)

The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in type Ia supernovae

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