Systematic trends in the motions of suspected stellar companions

Details Systematic trends in the motions of suspected stellar companions Systematic trends in the motions of suspected stellar companions

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mnras.175..533h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 175, June 1976, p. 533-535.

Astronomy and Astrophysics

Astronomy

11

Orbital Elements, Position Errors, Star Distribution, Stellar Motions, Astronomical Spectroscopy, Orbital Mechanics, Periodic Functions

Scientific paper

It is noted that orbital elements presented as evidence of unseen companions of certain stars have an unlikely distribution with respect to high inclinations. This distribution is shown to be a result of systematic errors in micrometric separations. The elements of the star BD +4 deg 3561 are examined, and no evidence for a real periodic motion is found.

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