Hot stars in old stellar populations: A continuing need for intermediate ages

Monthly Notices of the Royal Astronomical Society

Volumn 362, Issue 1, 2005, Pages 2-8

  Trager, S C ^a   Worthey, Guy ^b   Faber, S M ^c   Dressler, Alan ^d  

^a UNIVERSITY OF GRONINGEN   (Netherlands)

^b WASHINGTON STATE UNIVERSITY   (United States)

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

^d CARNEGIE OBSERVATORIES   (United States)

Author keywords

Galaxies: clusters: individual: Coma; Galaxies: elliptical and lenticular, cD; Galaxies: stellar content

Indexed keywords

METALS; STARS;

ABSORPTION LINES; BALMER LINES; EARLY TYPES; GALAXIES: CLUSTERS: INDIVIDUAL: COMA; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXY:STELLAR CONTENT; LINE STRENGTH; METAL ABSORPTION; METAL-POOR STAR; STELLAR POPULATIONS;

GALAXIES;

EID: 24944536210     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09288.x     Document Type: Article

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