OH maser emission from warm variable stars

Details OH maser emission from warm variable stars OH maser emission from warm variable stars

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...287l..35f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X), vol. 287, Dec. 1, 1984, p. L35-L37.

Astronomy and Astrophysics

Astrophysics

11

Hot Stars, Hydroxyl Emission, Interstellar Masers, Stellar Radiation, Variable Stars, Stellar Envelopes, Stellar Spectra

Scientific paper

Main line (1665 MHz/1667 MHz) OH emission from three warm variable stars, TW Aql, TX Per, and RV Tau, has been discovered. These stars are spectral class G when they are warmest and are considerably hotter than nearly all known stellar masers. The discovery of maser emission from these stars greatly enlarges the range of stellar types from which maser emission is observed.

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