Abstract
We have identified a candidate ∼1-2 × 105 yr 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 M⊙.
| Original language | English (US) |
|---|---|
| Pages (from-to) | L53-L56 |
| Journal | Astrophysical Journal |
| Volume | 499 |
| Issue number | 1 PART II |
| DOIs | |
| State | Published - 1998 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
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