Abstract
The nature of the peculiar emission properties of the T Tauri stars is examined in the light of contributions from regions designated as photospheres, chromosphere coronae, and extended envelopes which are often characterized by mass loss. Although some manifestations of T Tauri activity can be linked to vigorous solar-stellar phenomena characteristic of cool stars of low mass, other characteristics of T Tauri behavior are exhibited by a wide range of young stellar objects.
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Edwards, S., Strom, S.E. (1984). Recent observations of T Tauri stars. In: Baliunas, S.L., Hartmann, L. (eds) Cool Stars, Stellar Systems, and the Sun. Lecture Notes in Physics, vol 193. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-12907-3_174
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DOI: https://doi.org/10.1007/3-540-12907-3_174
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