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Constraining the Initial Mass Function via Stellar Transients

Constraining the Initial Mass Function via Stellar Transients

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_a01e5092a34048488b719e2de200667f

Constraining the Initial Mass Function via Stellar Transients

About this item

Full title

Constraining the Initial Mass Function via Stellar Transients

Publisher

Basel: MDPI AG

Journal title

Universe (Basel), 2024-10, Vol.10 (10), p.383

Language

English

Formats

Publication information

Publisher

Basel: MDPI AG

More information

Scope and Contents

Contents

The stellar initial mass function (IMF) represents a fundamental quantity in astrophysics and cosmology describing the mass distribution of stars from low mass all the way up to massive and very massive stars. It is intimately linked to a wide variety of topics, including stellar and binary evolution, galaxy evolution, chemical enrichment, and cosm...

Alternative Titles

Full title

Constraining the Initial Mass Function via Stellar Transients

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_a01e5092a34048488b719e2de200667f

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_a01e5092a34048488b719e2de200667f

Other Identifiers

ISSN

2218-1997

E-ISSN

2218-1997

DOI

10.3390/universe10100383

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