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Keck Interferometer Observations of Classical and Weak‐line T Tauri Stars
2005
Astrophysical Journal
We present observations of the T Tauri stars BP Tau, DG Tau, DI Tau, GM Aur, LkCa 15, RW Aur and V830 Tau, using long baseline infrared interferometry at K band (2.2 microns) from the Keck Interferometer. The target sources have a range of mass accretion rates and excess near-infrared emission. The interferometer is most sensitive to extended emission on characteristic size scales of 1 to 5 millarcseconds. All sources show evidence for resolved K band emission on these scales, although a few of
doi:10.1086/497436
fatcat:77e2uyl2gjamneangigrzletsu