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- W2034791031 abstract "This paper reports the detection of HDE 283572, a ninth-magnitude G star 8 arcmin south of RY Tau, as a bright X-ray source. The observations reveal this object to be a fairly massive (about 2 solar masses) pre-main-sequence star associated with the Taurus-Auriga star formation complex. It exhibits few of the characteristics of the classical T Tauri stars and is a good example of a 'naked' T Tauri star. The star is a mid-G subgiant, of about three solar radii and rotates with a period of 1.5 d. The coronal and chromospheric surface fluxes are similar to those of the most active late type stars (excluding T Tauri stars). The X-ray and UV lines most likely arise in different atmospheric structures. Radiative losses are some 1000 times the quiet solar value and compare favorably with those of T Tauri stars." @default.
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- W2034791031 date "1987-03-01" @default.
- W2034791031 modified "2023-09-28" @default.
- W2034791031 title "X-ray sources in regions of star formation. II - The pre-main-sequence G star HDE 283572" @default.
- W2034791031 doi "https://doi.org/10.1086/165059" @default.
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