Determination of the rotational excitation temperature in solar type stars

Details Determination of the rotational excitation temperature in solar type stars Determination of the rotational excitation temperature in solar type stars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..87...81f&link_type=abstract

Astrophysics and Space Science, vol. 87, no. 1-2, Oct. 1982, p. 81-87.

Astronomy and Astrophysics

Astrophysics

1

Hydroxyl Radicals, Molecular Excitation, Molecular Rotation, Molecular Spectra, Stellar Spectra, High Resolution, Iue, Line Spectra, Sun, Ultraviolet Spectra

Scientific paper

The OH molecular spectrum has been identified in three solar type stars,
Beta Com, Beta CVn, and Kappa Cet. The rotational excitation temperature
from molecular line intensities of OH has been determined for these
stars. The observations in high resolution were made by use of the IUE
satellite.

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