T-Tauri stars - Survey of observations and interpretation attempts

Details T-Tauri stars - Survey of observations and interpretation attempts T-Tauri stars - Survey of observations and interpretation attempts

May 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976s%26w....15..151b&link_type=abstract

Sterne und Weltraum, vol. 15, May 1976, p. 151-155. In German.

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Stellar Evolution, Stellar Spectra, T Tauri Stars, Absorption Spectra, Balmer Series, Classifications, Emission Spectra, H Alpha Line, Hertzsprung-Russell Diagram, Spatial Distribution, Spectrum Analysis, Star Distribution

Scientific paper

The stars considered were first defined with respect to their characteristics as members of a special group by Joy (1945, 1949). They are found in regions which exhibit intense dust absorption properties. Their space density is relatively high. The stars must be considered as young. Their study can, therefore, provide important information concerning the early phases of stellar development. The general characteristics of the stars are discussed, taking into account stellar classification, spectral properties, and an interpretation of the spectra. Attention is also given to details regarding the stage of development reached by the stars.

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