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 105 year old luminous white dwarf in NGC 1818, a young star cluster in the Large Magellanic Cloud. This discovery strongly constrains the boundary mass Mc at which stars stop forming neutron stars and start forming white dwarfs, to Mc > 7.6 Msun.
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