Superhump and outburst activity of the cataclysmic variable RZ LMi in the U- and optical passbands View Full Text


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Article Info

DATE

2018-05

AUTHORS

S. Y. Shugarov, N. A. Katysheva, D. Chochol, V. N. Krushevska, O. V. Vozyakova

ABSTRACT

An analysis of the new U,B,V,RC,IC-photometry of the cataclysmic variable RZ LMi obtained in 2016–17 showed the largest (U−B) colour excess in quiescence as well as during the decline of brightness, associated with the outbursts activity. The smallest (U−B) colour excess was found during the brightness increase from the quiescence. In contrast to the (U−B) colour index, the (B−V),(V−RC),(RC−IC) colour indices exhibits the largest colour excesses near the maximum of the outburst and the smallest during the quiescence. The (B−V) colour index showed also a large excess 1–2 days before a minimum. The detailed study of superhumps during the maximum of activity reveals the largest (U−B) colour excess at the time of the minimum brightness of superhumps. The (B−RC) colour index exhibits a similar behaviour, but with a phase shift of +0.1–+0.2 period of superhumps. The tracks in two-colour and colour-magnitude diagrams during superoutbursts are compared with the data for other cataclysmic variables during their outbursts as well as with published theoretical calculations. More... »

PAGES

100

References to SciGraph publications

  • 2002-10. Multicolor Photometry of Nova Lacertae 1910 = DI Lac in 1962-2002 in ASTROPHYSICS
  • 1984-01. UBV photometry and spectroscopy of an anomalous SS Cygni outburst in ASTROPHYSICS AND SPACE SCIENCE
  • 2008-06. Outbursts of selected dwarf novas and postnovas in BULLETIN OF THE CRIMEAN ASTROPHYSICAL OBSERVATORY
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    URI

    http://scigraph.springernature.com/pub.10.1007/s10509-018-3299-9

    DOI

    http://dx.doi.org/10.1007/s10509-018-3299-9

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