UV bright globular clusters in M87: More evidence for super-He-rich stellar populations?

Monthly Notices of the Royal Astronomical Society

Volumn 377, Issue 3, 2007, Pages 987-996

  Kaviraj, S ^a   Sohn, S T ^b,d   O'Connell, R W ^c   Yoon, S J ^d   Lee, Y W ^d   Yi, S K ^d  

^a UNIVERSITY OF OXFORD   (United Kingdom)

^b Korea Astronomy and Space Science Institute (KASI)   (South Korea)

^c UNIVERSITY OF VIRGINIA   (United States)

^d Yonsei University   (South Korea)

Author keywords

Galaxies: elliptical and lenticular, cD; Galaxies: evolution; Galaxies: formation; Galaxies: fundamental parameters; Globular clusters: general

Indexed keywords

GALAXIES; LUMINANCE; STARS;

CANONICAL MODELS; GALAXIES: ELLIPTICAL AND LENTICULAR CD; GALAXIES: FUNDAMENTAL PARAMETERS; GALAXY EVOLUTION; GALAXY FORMATIONS; GLOBULAR CLUSTERS; GLOBULAR CLUSTERS:GENERAL; HORIZONTAL BRANCHES; STELLAR POPULATIONS; WILKINSON MICROWAVE ANISOTROPY PROBE;

HELIUM;

EID: 34248158064     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.11712.x     Document Type: Article

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