Triple star systems nearer than 200 pc.

Details Triple star systems nearer than 200 pc. Triple star systems nearer than 200 pc.

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991bobeo.144...13p&link_type=abstract

Bulletin Astronomique de Belgrade, No. 144, p. 13 - 38

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Triple Systems: Surveys, Triple Systems: Nearby Stars, Triple Systems: Parallaxes

Scientific paper

A survey of 783 triple star systems is presented. All stars listed belong to the IDS Catalogue and are nearer than 200 pc. In addition to the system identification the survey includes SpA, πA and mA (main component), as well as the designation (multiple) of the apparent component configuration in the system. The data concerning the real relationship among the components (dynamical state) are also included; existence of orbits among the components, or a tendency for any orbital motion, is also specified. In order to examine the relationship between this survey on one side and the Leningrad Triple-Star-System Programme and Gliese's Nearby-Star Catalogue on the other side, suitable designations are brought in the survey. As a final step a short recapitulation of the survey data is done.

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