Testing the nature of S0 galaxies using planetary nebula kinematics in NGC 1023

Monthly Notices of the Royal Astronomical Society

Volumn 384, Issue 3, 2008, Pages 943-952

  Noordermeer, E ^a,k   Merrifield, M R ^a   Coccato, L ^b   Arnaboldi, M ^c   Capaccioli, M ^d   Douglas, N G ^e   Freeman, K C ^f   Gerhard, O ^b   Kuijken, K ^g   De Lorenzi, F ^b   Napolitano, N R ^h   Romanowsky, A J ^i,j  

^a UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^b MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d UNIVERSITY OF NAPLES FEDERICO II   (Italy)

^e UNIVERSITY OF GRONINGEN   (Netherlands)

^f AUSTRALIAN NATIONAL UNIVERSITY   (Australia)

^g LEIDEN UNIVERSITY   (Netherlands)

^h INAF OSSERVATORIO ASTRONOMICO DI CAPODIMONTE   (Italy)

ⁱ University of California Santa Cruz   (United States)

^j UNIVERSITY OF CONCEPCIÓN   (Chile)

^k NONE   (Netherlands)

more..

Author keywords

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

Indexed keywords

KINEMATICS; STARS;

GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES: INDIVIDUALS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES:STRUCTURE; GALAXY EVOLUTION; GALAXY: INDIVIDUAL: NGC 1023; GALAXY: INDIVIDUAL: NGC 1023A; PLANETARY NEBULA; SPIRAL GALAXIES;

GALAXIES;

EID: 43049146159     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12809.x     Document Type: Article

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