Significant evolution of the stellar mass-metallicity relation since z ∼ 0.65

Astronomy and Astrophysics

Volumn 447, Issue 1, 2006, Pages 113-119

  Liang, Y C ^a,b   Hammer, F ^b   Flores, H ^b  

^a CHINESE ACADEMY OF SCIENCES   (China)

^b UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Galaxies: abundances; Galaxies: evolution; Galaxies: ISM; Galaxies: spiral; Galaxies: starburst; Galaxies: stellar content

Indexed keywords

COSMIC RAYS; MAGNETIC FIELDS; OPTICAL TELESCOPES; SURVEYING INSTRUMENTS;

GALAXIES: ABUNDANCES; GALAXIES: EVOLUTION; GALAXIES: ISM; GALAXIES: SPIRAL; GALAXIES: STARBURST; GALAXIES: STELLAR CONTENT;

GALAXIES;

EID: 32544446957     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20053821     Document Type: Article

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