Computer Science
Scientific paper
Aug 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1158..223j&link_type=abstract
EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP Conference Proceedings, V
Computer Science
Origin And Evolution, Main-Sequence: Intermediate-Type Stars, Charge-Coupled Devices, Image Detectors, And Ir Detector Arrays
Scientific paper
At distances of only 3.3 and 3.6 pc respectively, V Eri and V Ind are two of the closest solar-type stars. In addition, they both exhibit long-term radial velocity (RV) trends indicative of planetary companions at relatively large separations, making them interesting for the purpose of direct imaging. Previously, we have reported the results of a deep imaging campaign of V Eri at 4 microns, which, in combination with dynamical data, led to the exclusion of any planets more massive than 3 Mjup anywhere in the system. Here, we will briefly review those results, as well as the results using the same method for V Ind A, where the massive planet or low-mass brown dwarf implied by the RV trend was undetected, and similar constraints could be determined on the system parameters.
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