Can galaxy outflows and re-accretion produce a downsizing in the specific star-formation rate of late-type galaxies?

Monthly Notices of the Royal Astronomical Society

Volumn 404, Issue 3, 2010, Pages 1100-1110

  Firmani, C ^a   Avila Reese, V ^a   Rodriguez Puebla A ^b  

^a INAF OSSERVATORIO ASTRONOMICO DI BRERA   (Italy)

^b UNIVERSIDAD NACIONAL AUTÓNOMA DE MÉXICO   (Mexico)

Author keywords

Cosmology: theory; Galaxies: evolution; Galaxies: haloes; Galaxies: high redshift; Galaxies: spiral; Galaxies: stellar content

Indexed keywords

COSMOLOGY; STARS;

COLD DARK MATTERS; COSMOLOGY: THEORY; DISK GALAXIES; GALAXIES: SPIRALS; GALAXIES:HIGH-REDSHIFT; GALAXY EVOLUTION; GALAXY:HALO; GALAXY:STELLAR CONTENT; STAR FORMATION RATES; STELLAR MASS;

GALAXIES;

EID: 77953573545     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.16366.x     Document Type: Article

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