The triple star Zeta Aquarii

Details The triple star Zeta Aquarii The triple star Zeta Aquarii

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...284..806h&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 284, Sept. 15, 1984, p. 806-809.

Astronomy and Astrophysics

Astrophysics

16

Companion Stars, Stellar Motions, Triple Stars, Angular Velocity, Orbital Position Estimation, Radial Velocity, Stellar Mass, Stellar Parallax, Visual Observation

Scientific paper

The accumulated data base of photographic plates of Zeta Aquarii are analyzed to verify the presence of a third companion and determine its physical and dynamic characteristics. A table of the relative orbital positions and residuals measured from 1781-1982 is provided. The masses of the stars are calculated to be 1.5, 0.4 and 1.5 solar mass, with the smallest star being fainter than 8 mag. A set of ephemerides is generated for 1982-2004.

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