The hydrogen emission of young stellar objects: key science for next-generation instruments and facilities

Details The hydrogen emission of young stellar objects: key science for next-generation instruments and facilities The hydrogen emission of young stellar objects: key science for next-generation instruments and facilities

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010spie.7734e..98g&link_type=abstract

Optical and Infrared Interferometry II. Edited by Danchi, William C.; Delplancke, Françoise; Rajagopal, Jayadev K. Proceeding

Physics

Scientific paper

The hydrogen emission line is a defining characteristic of young stellar objects probing the planet forming regions of the disks. The limiting sensitivity of current interferometers has precluded it's detailed study. We'll review our current understanding of hydrogen emission, recent results and project the science that can be achieved with sensitive interferometers such as the PRIMA off-axis mode and GRAVITY.

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