The 0.33 Day DA Plus DME Binary BPM 6502

Details The 0.33 Day DA Plus DME Binary BPM 6502 The 0.33 Day DA Plus DME Binary BPM 6502

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aj....120.3250k&link_type=abstract

The Astronomical Journal, Volume 120, Issue 6, pp. 3250-3254.

Astronomy and Astrophysics

Astronomy

14

Stars: Binaries: Close, Stars: Individual: Alphanumeric: Bpm 6502, Ultraviolet Emission, Stars: White Dwarfs

Scientific paper

We have obtained a series of spectroscopic measurements of the high proper-motion star BPM 6502 showing Balmer emission superposed upon the absorption lines. Radial velocity measurements determined by tracing optical absorption and emission lines show that the star is a binary system comprised of a DA white dwarf and an M dwarf with an orbital period of 0.33678 days. The space motion of the system falls within the general white dwarf population, and the system is not expected to initiate mass transfer within a Hubble time.

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