THE ORBITS OF THE TRIPLE-STAR SYSTEM 1 GEMINORUM FROM PHASES DIFFERENTIAL ASTROMETRY AND SPECTROSCOPY

We have used precise differential astrometry from the Palomar High-precision Astrometric Search for Exoplanet Systems project and radial-velocity measurements covering a time span of 40 yr to determine the orbital parameters of the 1 Geminorum triple system. We present the first detection of the spe...

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Veröffentlicht in:The Astrophysical journal 2014-03, Vol.783 (1), p.1-8
Hauptverfasser: Lane, Benjamin F, MUTERSPAUGH, MATTHEW W, Griffin, R F, Scarfe, C D, FEKEL, FRANCIS C, Williamson, Michael H, Eaton, Joel A, Shao, M, Colavita, M M, KONACKI, MACIEJ
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Sprache:eng
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Zusammenfassung:We have used precise differential astrometry from the Palomar High-precision Astrometric Search for Exoplanet Systems project and radial-velocity measurements covering a time span of 40 yr to determine the orbital parameters of the 1 Geminorum triple system. We present the first detection of the spectral lines of the third component of the system, together with precise mass (0.5%) and distance (0.15%) determinations for this system. In addition, our astrometry allows us to make the first determination of the mutual inclination of the orbits.
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/783/1/3