The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG

Details The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..140a&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Feb. 1989, p. 140-153. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

2

Hot Stars, Peculiar Stars, Stellar Evolution, Stellar Spectrophotometry, Symbiotic Stars, Ubv Spectra, Cygnus Constellation, Emission Spectra, Ionized Gases, Light Curve, Spectral Line Width, Stellar Color, Stellar Luminosity

Scientific paper

Photoelectric UBV observations of the peculiar eclipsing symbiotic star V1329 Cyg (HBV 475) were carried out during 1977-1988. After a single outburst in 1964, the star featured a light variation with the previous period of 950 d; however, the shape of the light curve changed and it began to resemble a sinusoid. The U-B and B-V color indices show that the radiation in the UBV bands is that of ionized gas most likely associated with a hot star.

Affiliated with

Also associated with

No associations

Rating

The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The photometric and spectral evolution of the peculiar symbiotic star V1329 CYG will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1885596