Effects of the radial flows on the chemical evolution of the Milky Way disk

Astronomy and Astrophysics

Volumn 531, Issue , 2011, Pages

  Spitoni, E ^a,c   Matteucci, F ^a,b  

^a UNIVERSITY OF TRIESTE   (Italy)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c UNIVERSITY OF ÉVORA   (Portugal)

Author keywords

Galaxy: abundances; Galaxy: disk; Galaxy: evolution; supernovae: general

Indexed keywords

CHEMICAL EVOLUTION; CONSTANT SPEED; GALACTIC DISKS; GALACTOCENTRIC DISTANCES; GALAXY: ABUNDANCES; GALAXY: DISK; GALAXY: EVOLUTION; GAS DENSITY; GAS FLOWS; GAS SPEED; METALLICITIES; MILKY WAYS; RADIAL INFLOW; STAR FORMATION RATES; STAR FORMATIONS; SUPERNOVAE: GENERAL; TIME-SCALES;

FLOW OF GASES; GALAXIES; GASES; RADIAL FLOW; STARS;

DENSITY OF GASES;

EID: 79958844465     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015749     Document Type: Article

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