arXiv · astro-ph/9802117
Discovery of a luminous white dwarf in a young star cluster in the Large Magellanic Cloud
Abstract
We have identified a candidate 1-2 x 10^5 year old luminous white dwarf in NGC 1818, a young star cluster in the Large Magellanic Cloud. This discovery strongly constrains the boundary mass M_c at which stars stop forming neutron stars and start forming white dwarfs, to M_c > 7.6 Msun.
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Rebecca A. W. Elson, Steinn Sigurdsson, Jarrod Hurley, Melvyn B. Davies, Gerard F. Gilmore. 1998-03-19. Discovery of a luminous white dwarf in a young star cluster in the Large Magellanic Cloud. https://doi.org/10.1086/311349
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