The fading of an extremely young T Tauri star and its associated nebula

Details The fading of an extremely young T Tauri star and its associated nebula The fading of an extremely young T Tauri star and its associated nebula

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978mnras.184..695c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 184, Sept. 1978, p. 695-698.

Astronomy and Astrophysics

Astronomy

5

M Stars, Nebulae, Stellar Luminosity, T Tauri Stars, Astronomical Photography, Emission Spectra, Line Spectra, Photosphere, Stellar Winds

Scientific paper

A faint M2 V star, showing a T Tau-like emission-line spectrum, has been
found in undistinguished dark cloud. The star is bright in the
near-infrared region and its location in the HR diagram suggests extreme
youth. The star had faded by about 1 mag between 1953 and 1954 as had an
arcuate cometary nebula associated with it.

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