A correlation between the H-alpha and SiO maser intensities of the long-period variable Chi Cygni

Details A correlation between the H-alpha and SiO maser intensities of the long-period variable Chi Cygni A correlation between the H-alpha and SiO maser intensities of the long-period variable Chi Cygni

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..461d&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, July-Aug. 1983, p. 461, 462) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, July

Astronomy and Astrophysics

Astronomy

H Alpha Line, Interstellar Masers, Radio Sources (Astronomy), Stellar Spectra, Variable Stars, Correlation, Cygnus Constellation, Millimeter Waves, Radiant Flux Density, Silicon Oxides

Scientific paper

The results of 1975 and 1978 - 79 observations of the Hα emission
line in the spectrum of χ Cyg are given. Comparison of the obtained
data with the observations of the SiO maser line (J = 2 - 1, v = 1) by
Wolff and Carlsson (1982) gives evidence of a correlation between the
intensities of the Hα and SiO lines.

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