Constraining the galaxy mass content in the core of A383 using velocity dispersion measurements for individual cluster members

Monthly Notices of the Royal Astronomical Society

Volumn 447, Issue 2, 2015, Pages 1224-1241

  Monna, A ^a,b   Seitz, S ^a,b   Zitrin, A ^c   Geller, M J ^d   Grillo, C ^e   Mercurio, A ^f   Greisel, N ^a,b   Halkola, A ^g   Suyu, S H ^h   Postman, M ⁱ   Rosati, P ^j   Balestra, I ^b,k   Biviano, A ^k   Coe, D ⁱ   Fabricant, D G ^d   Hwang, H S ^l   Koekemoer, A ⁱ  

^a UNIVERSITY OF MUNICH   (Germany)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

^e UNIVERSITY OF COPENHAGEN   (Denmark)

^f INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^g UNIVERSITY OF LÜBECK   (Germany)

^h INSTITUTE OF ASTRONOMY AND ASTROPHYSICS   (Taiwan)

ⁱ AURA for the European Space Agency   (United States)

^j UNIVERSITY OF FERRARA   (Italy)

^k INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^l Korea Institute for Advanced Study   (South Korea)

more..

Author keywords

A383 galaxies; Clusters; General galaxies; Gravitational lensing; Haloes dark matter; Individual; Strong galaxies

Indexed keywords

DISPERSIONS; GRAVITATION; IMAGE ENHANCEMENT; VELOCITY;

A383 - GALAXY; CLUSTER; DARK MATTER; GENERAL - GALAXIES; GRAVITATIONAL LENSING; HALO - DARK MATTER; INDIVIDUAL; STRONG - GALAXY; VELOCITY DISPERSION;

GALAXIES;

EID: 84922572717     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stu2534     Document Type: Article

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