A Substellar Companion with a Very Wide Separation from a Binary T Tauri Star

Details A Substellar Companion with a Very Wide Separation from a Binary T Tauri Star A Substellar Companion with a Very Wide Separation from a Binary T Tauri Star

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1158..253k&link_type=abstract

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY: Proceedings of the International Conference. AIP Conference Proceedings, V

Computer Science

Star Formation, Spectroscopy And Spectrophotometry, X-Ray Binaries

Scientific paper

We have conducted a high-resolution imaging and spectroscopic survey with the Subaru Telescope to study whether there is a maximum allowable separation of planetary-mass objects. It resulted in the detection of a possible planetary-mass (14 MJup) companion to a binary T Tauri star. The projected separation from its parent star is about 1,100 AU, the widest separation among planetary-mass companion candidates detected so far.

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