The most metal-poor damped Lyman α system at z < 3: Constraints on early nucleosynthesis

Astronomy and Astrophysics

Volumn 451, Issue 1, 2006, Pages 19-26

  Erni, P ^a   Richter, P ^a   Ledoux, C ^b   Petitjean, P ^c,d  

^a UNIVERSITY OF BONN   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^c CNRS   (France)

^d OBSERVATOIRE DE PARIS   (France)

Author keywords

Cosmology: early Universe; Cosmology: observations; Galaxies: abundances; Galaxies: quasars: absorption lines; Galaxies: quasars: individual: Q0913+072; Stars: formation

Indexed keywords

COSMIC RAYS; HYDROGEN; MATHEMATICAL MODELS; METALS; ULTRAVIOLET RADIATION;

COSMOLOGY: OBSERVATIONS; GALAXIES: QUASARS: ABSORPTION LINES; GALAXIES: QUASARS: INDIVIDUAL: Q0913+072; STARS: FORMATION;

GALAXIES;

EID: 33646535096     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20054328     Document Type: Article

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