期刊
ASTROPHYSICAL JOURNAL
卷 628, 期 1, 页码 L65-L68出版社
IOP PUBLISHING LTD
DOI: 10.1086/432540
关键词
circumstellar matter; infrared : stars; planetary systems : protoplanetary disks; stars : pre-main-sequence
We analyzed Spitzer Infrared Spectrograph data of a representative sample of classical T Tauri stars in the Taurus star-forming region by computing color indices in wave bands that characterize the continuum emission from dust in circumstellar disks. We compared these indices to those derived from a grid of accretion disk models with varying inclination angles, mass accretion rates, and amounts of dust settling. We conclude that most T Tauri stars in our sample have experienced some degree of dust settling and grain growth in their disks, indicating disk evolution.
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