Probing the hot gas in Young Stellar Objects with VLTI/AMBER

Details Probing the hot gas in Young Stellar Objects with VLTI/AMBER Probing the hot gas in Young Stellar Objects with VLTI/AMBER

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf..537t&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper, I give a summary of the recent results obtained with
AMBER on spectro-interferometric observations of Herbig Ae/Be stars.
This summary is not exhaustive but representative of the unique
capabilities of AMBER to probe the hot circumstellar gas, in addition to
the usually observed dust near-infrared thermal emission.

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