Optical spectroscopy of the candidate luminous white dwarf in the young LMC cluster NGC1818
Monthly Notices of the Royal Astronomical Society(2008)
摘要
An optical spectrum of the Elson et al. candidate luminous white dwarf in the young LMC cluster NGC 1818 shows conclusively that it is not a degenerate star. A model atmosphere fit gives Teff≈31 500 K and log g≈4.4, typical of a normal main-sequence B star. However, if it is a true LMC member then the star is underluminous by almost 3 mag. Its position in the cluster colour-magnitude diagram also ...
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关键词
stars: evolution,white dwarfs,globular clusters: individual: NGC 1818,Magellanic Clouds
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