First IR-interferometric Study Of The Physical Properties Of The Supergiant IRS 7 In The Particular Environment Of The Galactic Center.

Details First IR-interferometric Study Of The Physical Properties Of The Supergiant IRS 7 In The Particular Environment Of The Galactic Center. First IR-interferometric Study Of The Physical Properties Of The Supergiant IRS 7 In The Particular Environment Of The Galactic Center.

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21320407p&link_type=abstract

American Astronomical Society, AAS Meeting #213, #204.07; Bulletin of the American Astronomical Society, Vol. 41, p.267

Astronomy and Astrophysics

Astronomy

Scientific paper

The first successful observations with an optical long baseline interferometer of a supergiant in the Galactic center will be presented. GCIRS 7 is resolved by the VLTI baselines at 2 and 10microns. Its interaction with its particular environment can be studied. The unique L-band capabilities of the Keck interferometer promise to give further insights in the life of a star under influence of a supermassive black hole.

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