Paper:	Binaries in the Hipparcos Data: Keep Digging, II. Modeling the IAD of Known Spectroscopic Systems
Volume:	318, Spectroscopically and Spatially Resolving the Components of Close Binary Stars
Page:	144
Authors:	Pourbaix, D.; Jancart, S.; Jorissen, A.
Abstract:	We reprocess the Hipparcos Intermediate Astrometric Data of know spectroscopic binaries (retrived from the 9th catalogue of spectroscopic binary orbits, http://sb9.astro.ulb.ac.be) to see whether the orbital inclination, and thus the mass of the secondary, can be derived. Several statistical tests (Pourbaix & Arenou 2001) are used to ensure the reliability of the fit. About 70 systems (originally processed as single stars) out of 863 benefit from the orbital model.

Astronomical Society of the Pacific
Conference Series

© Copyright 1988 - 2024 - Astronomical Society of the Pacific
No part of the material protected by this copyright may be reproduced or used in any form other than for personal use without written permission from the ASP.

Page generated in 0.050 seconds