The evolution of the mass-metallicity relation in galaxies of different morphological types

Astronomy and Astrophysics

Volumn 504, Issue 2, 2009, Pages 373-388

  Calura, F ^a   Pipino, A ^b   Chiappini, C ^c,d   Matteucci, F ^a,d   Maiolino, R ^e  

^a UNIVERSITY OF TRIESTE   (Italy)

^b UNIVERSITY OF SOUTHERN CALIFORNIA   (United States)

^c UNIVERSITÉ DE GENÈVE   (Switzerland)

^d INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^e INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

Author keywords

Galaxies: abundances; Galaxies: high redshift; ISM: abundances

Indexed keywords

ABUNDANCE RATIOS; CHEMICAL EVOLUTION; ELLIPTICALS; FORMATION TIME; GALAXIES: ABUNDANCES; GALAXIES: HIGH-REDSHIFT; GALAXY FORMATIONS; ISM: ABUNDANCES; LONG LIFETIME; MASS DIAGRAMS; METALLICITIES; PHYSICAL MEANINGS; RED SHIFT; STAR FORMATION RATES; STAR FORMATIONS; ZERO POINT;

COSMOLOGY; DISPERSIONS; FORECASTING; METAL REFINING; MODELS; MORPHOLOGY; SMELTING;

GALAXIES;

EID: 70349339536     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200911756     Document Type: Article

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