Abstract
Optical spectroscopy of the extreme ultraviolet source EUVE J1439+75.0 revealed a new unresolved double degenerate system. The system is composed of two hot white dwarfs (Teff ≥ 20 000 K), one magnetic (∼10 MG) and the other apparently non-magnetic. Surface gravity measurements imply masses of ∼1.0 and ∼0.9 M⊙ for the magnetic and non-magnetic white dwarfs, respectively. Proposed radial velocity and spectro-polarimetric studies may help uncover evidence of past interactions and clarify the evolutionary status of the pair.
| Original language | English |
|---|---|
| Pages (from-to) | L49-L52 |
| Journal | Monthly Notices of the Royal Astronomical Society |
| Volume | 302 |
| Issue number | 3 |
| DOIs | |
| Publication status | Published - 21 Jan 1999 |
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