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SN 19841 - Another type Ib supernova
Publications of the Astronomical Society of the Pacific, 1990This object was discovered ~ 15 days before maximum light and was observed photometrically over a period of five weeks. A spectrum obtained near maximum shows that this supernova was a relatively distant Type-Ib event. Like other Type-Ib supernovae, 1984I was characterized by a red (B - V) color and low absolute magnitude at maximum.
B. Leibundgut +2 more
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Type Ib Supernovae Wolf-Rayet Stars
1991Since Type Ib supernovae were identified as a class several years ago, the idea that their progenitors are massive stars that have lost their hydrogen envelopes has been quite popular. ENSMAN and WOOSLEY [1] calculated a series of numerical models to test this idea and found that, if SNIb do come from massive stars (as opposed to, say, white dwarfs ...
Lisa Ensman, S. E. Woosley
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Type Ib and Ic Supernovae: Models and Spectra
1997For the theorist, Type Ib and Ic supernovae are the explosion of massive stars that have lost their hydrogen envelopes. For the observer, Type Ib supernovae are those that show no evidence of hydrogen, a weak or absent Si II absorption feature near 6150 A at peak light, and strong oxygen emission at late times.
S. E. Woosley, Ronald G. Eastman
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Type Ib supernovae: What they may be and what they are not
1988We show that the progenitors of Type Ib supernovae are likely to be moderately massive stars (M ∼ 7 M⊙) in binary systems and we argue that the hypothesis that they originate from very massive stars (M > 20 M⊙) is untenable both on an observational and a statistical basis.
Nino Panagia, Victoria G. Laidler
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Peculiar-Velocity Cosmology With Types Ia and II Supernovae
Monthly Notices of the Royal Astronomical Society, 2021Thomas de Jaeger +2 more
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Equations of State for Supernovae and Compact Stars
Reviews of Modern Physics, 2017Micaela Oertel, Stefan Typel
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Progenitors of Core-Collapse Supernovae
Annual Review of Astronomy and Astrophysics, 2009Stephen J. Smartt
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