Unravelling the origins of S0 galaxies using maximum likelihood analysis of planetary nebulae kinematics

Monthly Notices of the Royal Astronomical Society

Volumn 414, Issue 1, 2011, Pages 642-651

  Cortesi, A ^a,b   Merrifield, M R ^a   Arnaboldi, M ^b   Gerhard, O ^c   Martinez Valpuesta, I ^c   Saha, K ^c   Coccato, L ^c   Bamford, S ^a   Napolitano, N R ^d   Das, P ^c   Douglas, N G ^e   Romanowsky, A J ^f   Kuijken, K ^g   Capaccioli, M ^h   Freeman, K C ⁱ  

^a UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

^e UNIVERSITY OF GRONINGEN   (Netherlands)

^f University of California at Santa Cruz   (United States)

^g LEIDEN UNIVERSITY   (Netherlands)

^h UNIVERSITY OF NAPLES FEDERICO II   (Italy)

ⁱ AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

Author keywords

Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: individual: NGC 1023; Galaxies: individual: NGC 1023A; Galaxies: kinematics and dynamics

Indexed keywords

KINEMATICS; MAXIMUM LIKELIHOOD ESTIMATION; STARS;

GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES: INDIVIDUALS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY EVOLUTION; GALAXY: INDIVIDUAL: NGC 1023; GALAXY: INDIVIDUAL: NGC 1023A; MAXIMUM LIKELIHOOD ANALYSIS; PLANETARY NEBULA; STELLAR KINEMATICS;

GALAXIES;

EID: 79957911694     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18429.x     Document Type: Article

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