Star formation and chemical evolution of damped Lyman a systems

Monthly Notices of the Royal Astronomical Society

Volumn 322, Issue 4, 2001, Pages 927-932

  Ma, J ^a,b,c   Shu, C G ^b,d  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^d MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxies: stellar content

Indexed keywords

DENSITY OF GASES; GALAXIES; METALS; STARS;

BOX MODELS; CHEMICAL EVOLUTION; DISK GALAXIES; GALAXY EVOLUTION; GALAXY FORMATIONS; GALAXY:STELLAR CONTENT; METALLICITIES; RED SHIFT; SCHMIDT; STARS FORMATION;

ASTROPHYSICS;

EID: 0041819331     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2001.04199.x     Document Type: Article

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