The implications of the new Z = 0 stellar models and yields on the early metal pollution of the intergalactic medium

Astrophysical Journal

Volumn 557, Issue 1 PART 1, 2001, Pages 126-136

  Abia, C ^a   Dominguez I ^a   Straniero, O ^b   Limongi, M ^c   Chieffi, A ^d   Isern, J ^e  

^a UNIVERSITY OF GRANADA   (Spain)

^b INAF OSSERVATORIO ASTRONOMICO DI COLLURANIA   (Italy)

^c INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^d INAF IASF ROMA   (Italy)

^e INSTITUT D ESTUDIS ESPACIALS DE CATALUNYA IEEC   (Spain)

Author keywords

Galaxies: abundances; Galaxies: formation; Galaxies: intergalactic medium; Nuclear reactions, nucleosynthesis, abundances; Stars: luminosity function, mass function

Indexed keywords

EID: 0035839332     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/321660     Document Type: Article

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