Disc heating: Comparing the Milky Way with cosmological simulations

Monthly Notices of the Royal Astronomical Society

Volumn 415, Issue 3, 2011, Pages 2652-2664

  House, E L ^a   Brook, C B ^a   Gibson, B K ^a   Sanchez Blazquez P ^a,b   Courty, S ^a,c   Few, C G ^a   Governato, F ^d   Kawata, D ^e   Roskar R ^d,f   Steinmetz, M ^g   Stinson, G S ^a   Teyssier, R ^f,h  

^a UNIVERSITY OF CENTRAL LANCASHIRE   (United Kingdom)

^b UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^c CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^d UNIVERSITY OF WASHINGTON   (United States)

^e UNIVERSITY COLLEGE LONDON   (United Kingdom)

^f UNIVERSITY OF ZURICH   (Switzerland)

^g ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^h UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

Galaxies: evolution; Galaxies: formation; Galaxy: disc

Indexed keywords

CODES (SYMBOLS); DISPERSIONS; FLUID DYNAMICS; HEATING; MERGING; STARS;

DISC STARS; GALAXY EVOLUTION; GALAXY FORMATIONS; GALAXY: DISKS; GRID-BASED; MILKY WAYS; MODELLING TECHNIQUES; OBSERVATIONAL DATA; PROPERTY; STELLAR DISKS;

GALAXIES;

EID: 79961032624     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18891.x     Document Type: Article

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