Slow brightness variations of the peculiar object M1-2 = VV8 during 1971-1987

Details Slow brightness variations of the peculiar object M1-2 = VV8 during 1971-1987 Slow brightness variations of the peculiar object M1-2 = VV8 during 1971-1987

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..510a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, June 1988, p. 510-513. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Emission Spectra, Light Curve, Line Spectra, Peculiar Stars, Variable Stars, Astronomical Catalogs, Electrophotometry, Ubv Spectra

Scientific paper

Slow variations of the brightness and color indices of a starlike object
with M1-2 = VV8 emission lines were found on the basis of photoelectric
UBV observations carried out in 1971-1987. The amplitude in the V band
is determined to be about 0.2 m. It is suggested that these brightness
variations may be due to the reflection effect in a wide binary system.

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