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Results are presented for the He emission in 31 CTTS from the Taurus-Auriga molecular cloud spanning two orders of magnitude in the mass accretion rate, and for the Fe emission in DR Tau, based on a s...
High-resolution spectroscopy of classical T Tauri stars (CTTS) at one micron yields new insight into the interaction of accretion disks, outflowing gas, and the central stars. Eighty-one 0.95–1.12 μm ...
Are T Tauri stars gamma-ray emitters?     Tauri  stars  gamma-ray  emitters       2011/9/27
T Tauri stars are young, low mass, pre-main sequence stars surrounded by an accretion disk. These objects present strong magnetic activity and powerful magnetic reconnection events. Strong shocks are ...
Long-term, uniform series of UBVR observations of T Tauri and Herbig Ae stars obtained over 20 yr at the Maidanak Observatory as part of the ROTOR program are analyzed. We find a linear relationship...
Ultraviolet observations of classical T Tauri Stars (cTTSs) have shown that there is a hot (Te ≃ 80, 000 K) and dense (ne ≃ 1010 cm−3) component associated with the large scale jet. ...
We perform local excitation calculations to obtain line opacities and emissivity ratios and compare them with observed properties of H, He I, O I, Ca II, and Na I lines to determine the density, tempe...
Mass determination for T Tauri stars from JHK photometry。
New T Tauri Stars Associated with IRAS 05555-1405。
An empirical criterion to classify T Tauri stars and substellar analogs using low-resolution spectroscopy。
Magnetic Accretion Onto T Tauri Stars
Disks Around Classical T Tauri Stars     T Tauri Stars  Disks       2009/6/9
Disks Around Classical T Tauri Stars

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