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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

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Röpke,  F. K.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Hillebrandt,  W.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Röpke, F. K., & Hillebrandt, W. (2004). The case against the progenitor's carbon-to-oxygen ratio as a source of peak luminosity variations in type Ia supernovae. Astronomy & Astrophysics, 420(1), L1-L4. doi:10.1051/0004-6361:20040135.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0011-B66B-E
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