(Q56061263)

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Can Differences in the Nickel Abundance in Chandrasekhar‐Mass Models Explain the Relation between the Brightness and Decline Rate of Normal Type Ia Supernovae?

scientific article published in the Astrophysical Journal

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title

Can Differences in the Nickel Abundance in Chandrasekhar‐Mass Models Explain the Relation between the Brightness and Decline Rate of Normal Type Ia Supernovae? (English)

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Enrico Cappellaro

3

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author name string

Paolo A. Mazzali

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1

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Ken’ichi Nomoto

series ordinal

2

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Takayoshi Nakamura

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4

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Hideyuki Umeda

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5

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Koichi Iwamoto

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6

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language of work or name

English

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publication date

February 2001

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full work available at URL

https://iopscience.iop.org/article/10.1086/318428/pdf

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published in

The Astrophysical Journal

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volume

547

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issue

2

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page(s)

988–994

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ResearchGate publication ID

2225130

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(Q56061263)

Can Differences in the Nickel Abundance in Chandrasekhar‐Mass Models Explain the Relation between the Brightness and Decline Rate of Normal Type Ia Supernovae?

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