Masers associated with two carbon stars - V778 Cygni and EU Andromedae

Details Masers associated with two carbon stars - V778 Cygni and EU Andromedae Masers associated with two carbon stars - V778 Cygni and EU Andromedae

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...330..828l&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 330, July 15, 1988, p. 828-834.

Astronomy and Astrophysics

Astronomy

44

Carbon Stars, Hydroxyl Emission, Stellar Envelopes, Stellar Spectra, Water Masers, Binary Stars, Infrared Astronomy Satellite, M Stars, Maser Outputs

Scientific paper

The authors present several observations of the 22.2 GHz H2O maser line from two C stars, V778 Cyg and EU And, and the 1665/67 MHz OH maser lines from V778 Cyg. For both sources the intensity of the H2O line has varied by more than a factor of 5 over several months. The authors interpret the systems as being binaries, each with an M star component with a thick shell and a C star component.

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