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Empirically Derived Dynamical Models for the 55 Cancri and GJ 876 Planetary Systems

Published online by Cambridge University Press:  05 January 2015

Benjamin E. Nelson ,
Eric B. Ford ,
Jason T. Wright  and
Debra A. Fischer
Benjamin E. Nelson
Affiliation:
Dept. of Astronomy & Astrophysics, Pennsylvania State University Center for Exoplanets and Habitable Worlds 525 Davey Laboratory, University Park, Pennsylvania, USA, 16803 email: benelson@psu.edu
Eric B. Ford
Affiliation:
Dept. of Astronomy & Astrophysics, Pennsylvania State University Center for Exoplanets and Habitable Worlds 525 Davey Laboratory, University Park, Pennsylvania, USA, 16803 email: benelson@psu.edu
Jason T. Wright
Affiliation:
Dept. of Astronomy & Astrophysics, Pennsylvania State University Center for Exoplanets and Habitable Worlds 525 Davey Laboratory, University Park, Pennsylvania, USA, 16803 email: benelson@psu.edu
Debra A. Fischer
Affiliation:
Dept. of Astronomy, Yale University, New Haven, CT 06520USA
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Abstract

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In this paper we present empirically derived dynamical models for the 55 Cancri and GJ 876 planetary systems.

Keywords

planets and satellites: individual (55 Cancri; GJ 876)radial velocity
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S310: Complex Planetary Systems , July 2014 , pp. 93 - 95
Copyright
Copyright © International Astronomical Union 2014 

References

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