Do T-Tauri Stars have Extensive Coronae

Details Do T-Tauri Stars have Extensive Coronae Do T-Tauri Stars have Extensive Coronae

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981msngr..25...19k&link_type=abstract

The Messenger, No.25, P. 19, 1981

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Scientific paper

T Tauri stars are low-mass (= 3 M0 pre-main-sequence stars. They have been recognized the first time as an individual group of stars in 1945 by Alfred Joy. They show irregular photometrie variability and are located without exception in, or very close to, dark clouds. In 1958 another pioneer of variablestar research, George Herbig, proposed a number of spectroscopic criteria:

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