Cyclic Variations of T-Tauri Stars

Details Cyclic Variations of T-Tauri Stars Cyclic Variations of T-Tauri Stars

Mar 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981msngr..23...18k&link_type=abstract

The Messenger, No.23, P. 18, 1981

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

During a photographic survey of the Chamaeleon T association in 1971/72, evidence was found by Mauder and Sosna (Information Bulletin on Variable Stars, 1049, 1975) for quasi-cyclic light and colour variations of three variable stars, members of this nearby group of young stars. They were classified by Hoffmeister (Veröff. Sonneberg 6, 1, 1963) as T Tauri stars because of their light variations, and this type was confirmed with objective prism spectra by Henize and Mendoza (Astrophysical Journal, 180, 115, 1973).

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