VRI Photometry of Late Dwarf Common Proper-Motion Stars

Details VRI Photometry of Late Dwarf Common Proper-Motion Stars VRI Photometry of Late Dwarf Common Proper-Motion Stars

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..223w&link_type=abstract

Astrophysics and Space Science, Volume 142, Issue 1-2, pp. 223-225

Astronomy and Astrophysics

Astrophysics

Scientific paper

From the photometric observations of a sample of late dwarf common
proper motion pairs it may be inferred that about 30% - 50% of such
systems contain one or more additional stellar components. A small
fraction of such systems have separations in excess of 5000 A.U.

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