Stars in which planetary systems can be sought

Details Stars in which planetary systems can be sought Stars in which planetary systems can be sought

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..20..128z&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 20, Apr.-June 1986, p. 128-133. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomical Catalogs, Extrasolar Planets, Planetary Mass, Planetary Systems, Star Distribution, Binary Stars, Infrared Spectra, Solar System, Stellar Spectrophotometry

Scientific paper

A catalog of 53 stars selected from the solar vicinity (10-parsec radius) represents a novel attempt at a search for planetary systems. Stars of the following classes were chosen: (1) stars of the spectral classes F5-G9; (2) stars with low-mass satellites, (3) all stars situated within a 10-light-year-radius, (4) wide binaries with intracomponent distances greater than 30 AU, and (5) stars with IR excesses. It is concluded that the discovery of planetary systems will provide important information in the search for extraterrestrial life.

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