Measuring the Physical Properties of Young Substellar Companions

Details Measuring the Physical Properties of Young Substellar Companions Measuring the Physical Properties of Young Substellar Companions

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lyot.confe..29l&link_type=abstract

Proceedings of the conference In the Spirit of Bernard Lyot: The Direct Detection of Planets and Circumstellar Disks in the 21s

Physics

Scientific paper

Young nearby stars are promising targets for direct imaging of planetary companions because substellar objects are brightest when they are young. I will use recent observations of young substellar companions (e.g., GQ Lup B, 2M 1207B, CHXR73B) to illustrate some of the challenges in measuring the physical properties of planetary companions that are directly imaged around young stars.

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