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Cited by 543

The DOI matches its Crossref record; 36 of the 36 references it cites were found in a registry or an index.

The supernova rate per unit mass

Open access
Mannucci, F., Della Valle, M., Panagia, N., Cappellaro, E., Cresci, G., Maiolino, R., Petrosian, A., Turatto, M.·2005·Astronomy & Astrophysics

Abstract

We compute the rate of supernovae (SNe) of different types along the Hubble sequence normalized to the near-infrared luminosity and to the stellar mass of the parent galaxies. This is made possible by the new complete catalog of near-infrared galaxy magnitudes obtained by 2MASS. We find that the rates of all SN types, including Ia, Ib/c and II, show a sharp dependence on both the morphology and the () colors of the parent galaxies and, therefore, on the star formation activity. In particular we find, with a high statistical significance, that the type Ia rate in late type galaxies is a factor ~20 higher than in E/S0. Similarly, the type Ia rate in the galaxies bluer than is about a factor of 30 larger than in galaxies with . These findings can be explained by assuming that a significant fraction of Ia events in late spirals/irregulars originates in a relatively young stellar component.

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Metadata

Authors
Mannucci, F., Della Valle, M., Panagia, N., Cappellaro, E., Cresci, G., Maiolino, R., Petrosian, A., & Turatto, M.
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2005-03-29
Volume
433
Issue
3
Pages
807-814
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
OpenAlex
W2037095813
Cited by
543
References
36
FWCI
26.74
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The supernova rate per unit mass. https://app.cochat.ai/papers/10.1051/0004-6361:20041411
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Mannucci, F., Della Valle, M., Panagia, N., Cappellaro, E., Cresci, G., Maiolino, R., Petrosian, A., & Turatto, M. (2005). The supernova rate per unit mass. Astronomy & Astrophysics. https://doi.org/10.1051/0004-6361%3A20041411

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