Recent UBVR Photometry of Symbiotic Stars

We present recent photometric observations of Z And, BF Cyg, and AX Per made in the standard Johnson UBVR system. The main characteristics of their light behavior can be summarized as follows: Z And: our observations cover the recent active phase, from its maximum in 2000 December to the latest meas...

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Main Authors: Skopal A., Vaňko M., Pribulla T., Chochol D.
Format: Article
Language:English
Published: De Gruyter 2003-12-01
Series:Open Astronomy
Subjects:
Online Access:https://doi.org/10.1515/astro-2017-0095
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author Skopal A.
Vaňko M.
Pribulla T.
Chochol D.
author_facet Skopal A.
Vaňko M.
Pribulla T.
Chochol D.
author_sort Skopal A.
collection DOAJ
description We present recent photometric observations of Z And, BF Cyg, and AX Per made in the standard Johnson UBVR system. The main characteristics of their light behavior can be summarized as follows: Z And: our observations cover the recent active phase, from its maximum in 2000 December to the latest measurements (2003 September). BF Cyg: the minimum of the recent wave in the star’s brightness was the deepest ever observed; in 2003 February a short-term flare developed in the light curve. AX Per: from 1995 October the light curve displays signatures of a quiescent phase of the star; in 2003 May a 0.5 mag flare was detected.
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spelling doaj.art-a1df5a13d5e74e9f9220c68614f903f82022-12-21T22:38:59ZengDe GruyterOpen Astronomy2543-63762003-12-0112463163210.1515/astro-2017-0095astro-2017-0095Recent UBVR Photometry of Symbiotic StarsSkopal A.0Vaňko M.1Pribulla T.2Chochol D.3Astronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, SlovakiaAstronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, SlovakiaAstronomical Institute, Slovak Academy of Sciences, 059 60 Tatranská Lomnica, SlovakiaAstronomical Institute, Slovak Academy of Sciences, 059 60 Tatransá Lomnica, SlovakiaWe present recent photometric observations of Z And, BF Cyg, and AX Per made in the standard Johnson UBVR system. The main characteristics of their light behavior can be summarized as follows: Z And: our observations cover the recent active phase, from its maximum in 2000 December to the latest measurements (2003 September). BF Cyg: the minimum of the recent wave in the star’s brightness was the deepest ever observed; in 2003 February a short-term flare developed in the light curve. AX Per: from 1995 October the light curve displays signatures of a quiescent phase of the star; in 2003 May a 0.5 mag flare was detected.https://doi.org/10.1515/astro-2017-0095starsbinariessymbiotictechniquesphotometric
spellingShingle Skopal A.
Vaňko M.
Pribulla T.
Chochol D.
Recent UBVR Photometry of Symbiotic Stars
Open Astronomy
stars
binaries
symbiotic
techniques
photometric
title Recent UBVR Photometry of Symbiotic Stars
title_full Recent UBVR Photometry of Symbiotic Stars
title_fullStr Recent UBVR Photometry of Symbiotic Stars
title_full_unstemmed Recent UBVR Photometry of Symbiotic Stars
title_short Recent UBVR Photometry of Symbiotic Stars
title_sort recent ubvr photometry of symbiotic stars
topic stars
binaries
symbiotic
techniques
photometric
url https://doi.org/10.1515/astro-2017-0095
work_keys_str_mv AT skopala recentubvrphotometryofsymbioticstars
AT vankom recentubvrphotometryofsymbioticstars
AT pribullat recentubvrphotometryofsymbioticstars
AT chochold recentubvrphotometryofsymbioticstars