Discovery of 14 Nearby Double Stars

Details Discovery of 14 Nearby Double Stars Discovery of 14 Nearby Double Stars

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aj....121.3259m&link_type=abstract

The Astronomical Journal, Volume 121, Issue 6, pp. 3259-3265.

Astronomy and Astrophysics

Astronomy

12

Stars: Binaries: General

Scientific paper

We report the discovery of 14 double-star systems with main-sequence
primaries, most of which are M type. Infrared imaging indicates that the
secondaries are most likely late-type dwarfs. The fact that most of the
stars are within 25 pc underscores the incompleteness of our present
census of our nearest neighbors.

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