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Single-line spectroscopic binary

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Single-Line Spectroscopic Binary
A spectroscopic binary in which lines of one star are visible in the spectrum.
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According to the Yale Bright Star Catalogue, 1991 5th Revised Edition notes entry for HR 4785, a possible companion object was detected as a single-line spectroscopic binary with an estimated orbital period of 2,430 days.

See also: Luminosity Class, Constellations, Earth, Solar, Astronomy

Astronomy SilicatesSingularity

 
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