Determination of the rotational excitation temperature in solar type stars.
DOI: 10.1007/BF00648909
Bibcode: 1982Ap&SS..87...81F
Rego, M.; Fernandez-Figueroa, M. J.; Perea, A.
Spain
Abstract
The OH molecular spectrum has been identified in three solar type stars, β Com, β CVn, and κ 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.
1982
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Astrophysics and Space Science
IUE
1