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Planetary mass limits using Hipparcos astrometry

Published online by Cambridge University Press:  26 May 2016

Frédéric Arenou
Affiliation:
CNRS/Observatoire de Paris, France
Julienne Palasi
Affiliation:
CNRS/Observatoire de Paris, France

Abstract

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Using Hipparcos and Tycho-2 data, together with the radial velocity information, a statistical analysis is applied to all the orbital solutions of planetary candidates, in order to avoid a bias towards small inclinations. There are hints of additional, longer period companions.

Type
Part I: Discovery and study of extrasolar planets - current
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Fischer, D. et al. 2000, ApJ, submitted.Google Scholar
Halbwachs, J.L., Arenou, F., Mayor, M., Udry, S., Queloz, D. 2000, A&A 355, 581.Google Scholar
Høg, E., et al. 2000, A&A 355, 27.Google Scholar
Mazeh, T., Zucker, S., dalla Torre, A., van Leeuwen, F. 1999, ApJ 522, L149.CrossRefGoogle Scholar
Mazeh, T., et al., 2000, ApJ 532, 55.Google Scholar
Perryman, M.A.C. et al. 1996, A&A 310, L21.Google Scholar
Queloz, D. et al. 2000, A&A 354, 99.Google Scholar
Schneider, J. 2000, http://www.obspm.fr/planets, 1st August version.Google Scholar
Zucker, S., Mazeh, T. 2000, ApJ 531, 67.Google Scholar