Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995coska..25...53s&link_type=abstract
Contributions of the Astronomical Observatory Skalnate Pleso, Volume 25, p. 53-73
Astronomy and Astrophysics
Astronomy
17
Light Curve, Symbiotic Stars, Ubv Spectra, Astronomical Photometry, Visual Observation, Electrophotometry, Stellar Luminosity, Periodic Variations, Photographs, Histories
Scientific paper
We present new observations of 19 symbiotic and symbiotic-like stars. Photoelectric UBV(R) observations cover the 1993.75 to 1994.75 period. The main results can be summarized as follows: Z And: the visual light curve (LC) indicates a quiet stage of the star. EG And: The primary minimum at JD 2 449 230 was observed. V 1413 Aql: The recent outburst has probably finished. UV Aur: Historical photographic LC from December 1895 to March 1963 is presented. It suggests changes in the periodicity of the brightness variation being approximately between 395 and 360 days. TX CVn: A slow gradual decrease in the star's brightness is observed. Historical photographic LC from May 1906 to March 1992 is presented. It indicates an increase in the activity approximately at JD 2434000. T CrB: Observations indicate a decrease of brightness mainly in U. BF Cyg: The star has returned to quiescence. Historical photographic LC from October 1896 to September 1992 is presented.
Chochol Drahomir
Hric Ladislav
Komzik Richard
Niarchos Panagiotis
Oprescu Gabriela
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Photometry of symbiotic stars: an international campaign 6. Z and, EG and, V1413 AQL (AS 338), R Aqr, UV Aur, TX CVn, T CrB, BF Cyg, CH Cyg, CI Cyg, V 1016 Cyg, AG Dra, CQ DRA (4 Dra), YY Her, V 443 Her, SS Lep, AG Peg, AX Per, PU VUL does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
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