OH/H2O/SiO/IR stellar masers

Details OH/H2O/SiO/IR stellar masers OH/H2O/SiO/IR stellar masers

Dec 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mmsai..51..695p&link_type=abstract

(Società Astronomica Italiana, Convegno sulla Variabilita Stellare, 1st, Massalubrense, Italy, May 22-24, 1980.) Società Astrono

Astronomy and Astrophysics

Astronomy

Hydroxyl Emission, Infrared Stars, Masers, Radio Stars, Silicon Oxides, Stellar Radiation, Stellar Spectra, Infrared Spectra, M Stars, Radial Velocity, Semiregular Variable Stars, Spectral Energy Distribution, Supergiant Stars, Variable Stars, Water Vapor

Scientific paper

The main infrared and radio properties of the stellar masers OH, H2O and
SiO are reviewed. Maser emission in the three molecules is observed
almost exclusively in M-type Miras with mean spectral types later than
M5 and pulsation period greater than 200 days, semiregular variables,
and M-supergiants of spectral types as early as M3.

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