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Titolo:
Young clusters in the Magellanic Clouds. II
Autore:
Keller, SC; Da Costa, GS; Bessell, MS;
Indirizzi:
Australian Natl Univ, Inst Adv Studies, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia Australian Natl Univ Weston ACT Australia 2611 eston, ACT 2611, Australia
Titolo Testata:
ASTRONOMICAL JOURNAL
fascicolo: 2, volume: 121, anno: 2001,
pagine: 905 - 915
SICI:
0004-6256(200102)121:2<905:YCITMC>2.0.ZU;2-L
Fonte:
ISI
Lingua:
ENG
Soggetto:
EVOLUTIONARY MODELS; MASSIVE STARS; RADIATIVE OPACITIES; NGC-1866; NGC-330; SUPERGIANTS; SEQUENCES; DIAGRAMS;
Keywords:
galaxies : star clusters; Magellanic Clouds; stars : evolution;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Physical, Chemical & Earth Sciences
Citazioni:
33
Recensione:
Indirizzi per estratti:
Indirizzo: Keller, SC Univ Calif Lawrence Livermore Natl Lab, L-413,7000 East Ave, Livermore, CA94551 USA Univ Calif Lawrence Livermore Natl Lab L-413,7000 EastAve Livermore CA USA 94551
Citazione:
S.C. Keller et al., "Young clusters in the Magellanic Clouds. II", ASTRONOM J, 121(2), 2001, pp. 905-915

Abstract

We present the results of a quantitative study of the degree of extension to the boundary of the classical convective core within intermediate-mass stars. The basis of our empirical study is the stellar population of four young populous clusters in the Magellanic Clouds that has recently been detailed by Keller, Bessell, & Da Costa. The sample affords a meaningful comparison with theoretical scenarios with varying degrees of convective core overshoot and binary star fraction. Two critical properties of the population, the main-sequence luminosity function and the number of evolved stars, formthe basis of our comparison between the observed data set and that simulated from the stellar evolutionary models. On the basis of this comparison weconclude that the case of no convective core overshoot is excluded at a 2 sigma level.

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Documento generato il 20/06/13 alle ore 09:29:32