A study of broad-line OH emission sources - OH231.8+4.2, VY CMa, and M1-92

Details A study of broad-line OH emission sources - OH231.8+4.2, VY CMa, and M1-92 A study of broad-line OH emission sources - OH231.8+4.2, VY CMa, and M1-92

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980aj.....85..724m&link_type=abstract

Astronomical Journal, vol. 85, June 1980, p. 724-737.

Astronomy and Astrophysics

Astronomy

67

Emission Spectra, Hydroxyl Emission, Line Spectra, Nebulae, Astronomical Models, Energy Levels, Far Infrared Radiation, Masers, Periodic Variations

Scientific paper

The observations discussed represent a portion of a long-term project to
monitor the OH flux from a large number of OH/IR stars (Bowers, 1980).
Consideration is given to emission sources OH231.8+4.2, VY CMa, and
M1-92.

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