Precision Orbit of δ Delphini and Prospects for Astrometric Detection of Exoplanets

Gardner, Tyler, Monnier, John D., Fekel, Francis C., Williamson, Mike, Duncan, Douglas K., White, Timothy R., Ireland, Michael, Adams, Fred C., Barman, Travis, Baron, Fabien, ten Brummelaar, Theo, Che, Xiao, Huber, Daniel, Kraus, Stefan, Roettenbacher, Rachael M., Schaefer, Gail, Sturmann, Judit, Sturmann, Laszlo, Swihart, Samuel J., Zhao, Ming

Precision Orbit of δ Delphini and Prospects for Astrometric Detection of Exoplanets

The Astrophysical Journal, Volume 855, Issue 1

Abstract

Combining visual and spectroscopic orbits of binary stars leads to a determination of the full 3D orbit, individual masses, and distance to the system. We present a full analysis of the evolved binary system δ Delphini using astrometric data from the MIRC and PAVO instruments on the CHARA long-baseline interferometer, 97 new spectra from the Fairborn Observatory, and 87 unpublished spectra from the Lick Observatory. We determine the full set of orbital elements for δ Del, along with masses of 1.78 ± 0.07 M

Keywords: astrometry, binaries: close, binaries: spectroscopic, binaries: visual, planets and satellites: detection

Leave a Reply

Your email address will not be published. Required fields are marked *