Young Stellar Objects with the Keck Interferometer

Details Young Stellar Objects with the Keck Interferometer Young Stellar Objects with the Keck Interferometer

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.0709m&link_type=abstract

American Astronomical Society Meeting 203, #07.09; Bulletin of the American Astronomical Society, Vol. 35, p.1214

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Scientific paper

Here we report first results of a survey of young stellar objects (YSO) with the newly-commissioned Keck Interferometer (Keck-I). The Keck-I has an order-of-magnitude greater sensitivity than other near-infrared interferometers allowing characteristic size measurements of a wide variety of YSO systems. The inner accretion disks of Classical T Tauris, Herbig Ae/Be stars, and FU Orionis objects have been observed at astronomical K-band (2.2 microns) and nearly all targets were resolved. In this poster, we present a status report and preliminary analysis of our initial dataset.
This work has been funded by NASA. The interferometer observations were made possible through the efforts of the NASA-Jet Propulsion Laboratory, the W. M. Keck Observatory, and the Michelson Science Center (Caltech).

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