Metallicity gradients in disks: Do galaxies form inside-out?

Astronomy and Astrophysics

Volumn 540, Issue , 2012, Pages

  Pilkington, K ^a,b,c   Few, C G ^a,b   Gibson, B K ^a,b,c   Calura, F ^a,d   Michel Dansac, L ^e   Thacker, R J ^b   Molla M ^a,f   Matteucci, F ^g   Rahimi, A ^h   Kawata, D ^h   Kobayashi, C ⁱ   Brook, C B ^a,j   Stinson, G S ^a,k   Couchman, H M P ^l   Bailin, J ^m   Wadsley, J ^l  

^a UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^b SAINT MARY S UNIVERSITY   (Canada)

^c MONASH UNIVERSITY   (Australia)

^d OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^e UNIVERSITÉ LYON 1   (France)

^f CIEMAT   (Spain)

^g UNIVERSITY OF TRIESTE   (Italy)

^h UNIVERSITY COLLEGE LONDON   (United Kingdom)

ⁱ UNIVERSITY OF HERTFORDSHIRE   (United Kingdom)

^j UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^k MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^l MCMASTER UNIVERSITY   (Canada)

^m UNIVERSITY OF MICHIGAN   (United States)

more..

Author keywords

galaxies: abundances; galaxies: evolution; galaxies: formation; Galaxy: disk

Indexed keywords

ADAPTIVE MESH REFINEMENT CODES; CHEMICAL EVOLUTION; DISK GALAXIES; FUNCTION OF TIME; GALAXIES: ABUNDANCES; GALAXIES: EVOLUTIONS; GALAXIES: FORMATION; GALAXY SIMULATIONS; GALAXY: DISKS; HIGH-REDSHIFT; HOT SIMULATION; LATE-TYPE; METALLICITIES; MILKY WAYS; RADIAL GRADIENT; RATE OF CHANGE; RED SHIFT; SELF-SIMILARITIES; SMOOTHED PARTICLE HYDRODYNAMICS; SUB-GRIDS; TEMPORAL EVOLUTION; THICK DISK; THIN DISK;

ASTROPHYSICS; COMPUTER SIMULATION; FLUID DYNAMICS; STARS;

GALAXIES;

EID: 84859012054     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117466     Document Type: Article

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