Studying Star Formation with the Keck Interferometer

Details Studying Star Formation with the Keck Interferometer Studying Star Formation with the Keck Interferometer

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..221..301a&link_type=abstract

Star Formation at High Angular Resolution, International Astronomical Union Symposium 221, held during the XXV General Assembly

Astronomy and Astrophysics

Astronomy

Scientific paper

The Keck Interferometer utilizes the two 10-meter Keck telescopes as a direct detection interferometer in the infrared. The 85-meter baseline produces a fringe spacing of 5 milliarcseconds at 2 microns, or 0.7 AU for sources in the Taurus star forming region. The first observations with the Keck Interferometer of T Tauri and Herbig Ae/Be sources are presented and the implications for circumstellar disk models are discussed.

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