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

Paulo J. V. Garcia; Myriam Benisty; Samira Rajabi; Catherine Dougados; Fabrizzio Massi; Francesca Bacciotti; Jean-Baptiste Le Bouquin; Fabien Malbet; Linda Podio; Stephanie Renard; Emma Whelan

doi:10.1117/12.858302

21 July 2010 The hydrogen emission of young stellar objects: key science for next-generation instruments and facilities

Paulo J. V. Garcia, Myriam Benisty, Samira Rajabi, Catherine Dougados, Fabrizzio Massi, Francesca Bacciotti, Jean-Baptiste Le Bouquin, Fabien Malbet, Linda Podio, Stephanie Renard, Emma Whelan

Author Affiliations +

Proceedings Volume 7734, Optical and Infrared Interferometry II; 773434 (2010) https://doi.org/10.1117/12.858302
Event: SPIE Astronomical Telescopes + Instrumentation, 2010, San Diego, California, United States

Abstract

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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Paulo J. V. Garcia, Myriam Benisty, Samira Rajabi, Catherine Dougados, Fabrizzio Massi, Francesca Bacciotti, Jean-Baptiste Le Bouquin, Fabien Malbet, Linda Podio, Stephanie Renard, and Emma Whelan "The hydrogen emission of young stellar objects: key science for next-generation instruments and facilities", Proc. SPIE 7734, Optical and Infrared Interferometry II, 773434 (21 July 2010); https://doi.org/10.1117/12.858302

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