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The photometric observations of new WZ Sge-type systems with small telescopes

In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no. 3
N. Katysheva - D. Chochol - S. Shugarov
Detaily:
Rok, strany: 2014, 306 - 311
Kľúčové slová:
cataclysmic variables, dwarf novae, WZ Sge-stars— superoutbursts, superhumps, photometry
O článku:
The last few years have been marked by discoveries and studies of the powerful outbursts of the WZ Sge-type dwarf novae with small telescopes. These objects are characterized by very short orbital periods (mostly 80—90 min), strong and rare superoutbursts and very specific light curve features — superhumps. We carried out the multicolour observations of some WZ Sge-type systems during their superoutbursts, fadings, rebrightenings (if they were detected) and in quiescence using small telescopes (60-, 125-cm) of the Crimean station of Moscow State University and the Astromonical Institute of the Slovak Academy of Sciences. A short review of the WZ Sge-type objects, having been observed in these observatories, is presented. Possibility of good investigation of CVs with small telescopes, equipped with CCD-cameras, is very relevant.
Ako citovať:
ISO 690:
Katysheva, N., Chochol, D., Shugarov, S. 2014. The photometric observations of new WZ Sge-type systems with small telescopes. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 43, no.3, pp. 306-311. 1335-1842.

APA:
Katysheva, N., Chochol, D., Shugarov, S. (2014). The photometric observations of new WZ Sge-type systems with small telescopes. Contributions of the Astronomical Observatory Skalnaté Pleso, 43(3), 306-311. 1335-1842.