Band strengths of M stars in the Orion population

Details Band strengths of M stars in the Orion population Band strengths of M stars in the Orion population

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mnras.181..625m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 181, Dec. 1977, p. 625-635.

Astronomy and Astrophysics

Astronomy

13

M Stars, Spectral Line Width, Stellar Spectra, T Tauri Stars, Calcium Compounds, Hydrides, Main Sequence Stars, Molecular Spectra, Stellar Evolution, Stellar Gravitation, Titanium Oxides

Scientific paper

Narrow-band measurements of CaH and TiO band strengths are reported for
T Tauri stars of spectral type M. The observations imply a surface
gravity an order of magnitude below that of the lower main sequence,
consistent with the quasi-steady contractional evolution of low-mass
stars.

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