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On the Nature and Origin of the T Tauri Stars

Published online by Cambridge University Press:  14 August 2015

George H. Herbig
George H. Herbig*
Affiliation:
Lick Observatory, Mount Hamilton, California, U.S.A.

Extract

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It is fitting that, in opening this Symposium with a consideration of the T Tauri stars, we note that this month marks the tenth anniversary of the September 1945 issue of the Astrophysical Journal, in which appeared the remarkable pioneering paper by Alfred H. Joy that initiated the study of emission-line stars associated with nebulosity. This contribution opened a new approach to the study of the relationship of stars to their environment. Today, ten years later, the T Tauri stars and their interaction with nebular material form a topic whose significance we may not fully appreciate and whose opportunities have been as yet only superficially exploited.

Type
I. Instability in Dwarf Stars of Later Type: T Tauri Stars and Related Objects, and The UV Ceti Variables
Information
Symposium - International Astronomical Union , Volume 3: Non-Stable Stars , 1957 , pp. 3 - 10
Copyright
Copyright © Cambridge University Press 1957 

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