VRI photometry of late dwarf common proper motion pairs

Details VRI photometry of late dwarf common proper motion pairs VRI photometry of late dwarf common proper motion pairs

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....101.1882w&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 101, May 1991, p. 1882-1901.

Astronomy and Astrophysics

Astronomy

28

Astronomical Photometry, Dwarf Stars, Late Stars, Stellar Motions, Astronomical Catalogs, Binary Stars, Distance, M Stars

Scientific paper

VRI photometry and photometric distance moduli are presented for 266 late dwarf common proper motion pairs. From the distance modulus differences between the components of each pair, it is inferred that at least 56 percent of the pairs contain one or more additional stellar components. The maximum separation of M dwarf binaries appears to be of the order 10,000-20,000 AU.

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