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The Enrichment of the Intracluster Medium

Galactic Winds, Dwarf Galaxies, and Bimodal Star Formation in Ellipticals
descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 1996Embargo end date: 01 Jan 1996 English Publisher:Springer NetherlandsJournal:Symposium - International Astronomical Union, volume 171, pages 381-381 (issn: 0074-1809, Copyright policy )
Authors: Francesca Matteucci; Brad K. Gibson;

doi: 10.1007/978-94-009-0229-9_93 , 10.1017/s0074180900233007 , 10.48550/arxiv.astro-ph/9612131

arXiv: http://arxiv.org/abs/astro-ph/9612131

The Enrichment of the Intracluster Medium

Abstract

Recent observational evidence for steep dwarf galaxy luminosity functions in several rich clusters has led to speculation that their precursors, via supernovae (SNe)-driven galactic winds, may be the source of the majority of gas and metals inferred from intracluster medium (ICM) x-ray observations (Trentham 1994). Utilising a fully self-consistent photo-chemical evolution package (Gibson 1995), and insisting that the post-galactic wind dwarfs obey the observed colour-luminosity-metallicity relations, we demonstrate that the bulk of the ICM gas does not originate within their precursors (Gibson & Matteucci 1995).

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Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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citations
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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