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Characterizing the stellar photospheres and near-infrared excesses in accreting T Tauri systems

By M. Mcclure and others
Using NASA IRTF SpeX data from 0.8 to 4.5 \mum, we determine self-consistently the stellar properties and excess emission above the photosphere for a sample of classical T Tauri stars (CTTS) in the Taurus molecular cloud with varying degrees of accretion. This process uses a combination of techniques from the... Show more
March 30, 2013
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Characterizing the stellar photospheres and near-infrared excesses in accreting T Tauri systems
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