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Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-ric...

Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-ric...

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2724402607

Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-rich Type IIb Supernovae from the Zwicky Transient Facility

About this item

Full title

Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-rich Type IIb Supernovae from the Zwicky Transient Facility

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2023-10

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

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Scope and Contents

Contents

The fate of stars in the zero-age main-sequence (ZAMS) range \(\approx 8-12\) Msun is unclear. They could evolve to form white dwarfs or explode as electron-capture supernovae (SNe) or iron core-collapse SNe (CCSNe). Even though the initial mass function indicates that this mass range should account for over 40% of all CCSNe progenitors, few have b...

Alternative Titles

Full title

Probing the low-mass end of core-collapse supernovae using a sample of strongly-stripped Calcium-rich Type IIb Supernovae from the Zwicky Transient Facility

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Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2724402607

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2724402607

Other Identifiers

E-ISSN

2331-8422

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