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X-ray emission from T Tauri stars
Monthly Notices of the Royal Astronomical Society, no. 3 (2006): 917-927
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摘要
We have modelled the X-ray emission of T Tauri stars assuming that they have isothermal, magnetically confined coronae. These coronae extend outwards until either the pressure of the hot coronal gas overcomes the magnetic field, or, if the corona interacts with a disc before this happens, by the action of the disc itself. This work is mot...更多
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