Long-period Exoplanets And Brown Dwarfs From The California And Carnegie Planet Search

Details Long-period Exoplanets And Brown Dwarfs From The California And Carnegie Planet Search Long-period Exoplanets And Brown Dwarfs From The California And Carnegie Planet Search

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...210.0902w&link_type=abstract

American Astronomical Society Meeting 210, #09.02; Bulletin of the American Astronomical Society, Vol. 39, p.105

Astronomy and Astrophysics

Astronomy

Scientific paper

Some substellar companions to target stars in our radial velocity planet searches have periods much longer than the program's 10-15 y baseline. Since waiting for these objects to complete an orbit may be impractical, we have developed techniques for constraining their orbital elements with incomplete orbital information. These techniques have allowed us to identify new brown-dwarf companions, new exoplanets, and new multiple-planet systems.

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