Five-color photometry of DQ HER (N HER 1934). I

Details Five-color photometry of DQ HER (N HER 1934). I Five-color photometry of DQ HER (N HER 1934). I

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985afz....22...31d&link_type=abstract

(Astrofizika, vol. 22, Jan.-Feb. 1985, p. 31-42) Astrophysics (ISSN 0571-7132), vol. 21, no. 1, July 1985, p. 17-24. Translation

Astronomy and Astrophysics

Astrophysics

6

Cataclysmic Variables, Eclipsing Binary Stars, Light Curve, Novae, Stellar Spectrophotometry, White Dwarf Stars, Accretion Disks, Stellar Activity, Stellar Envelopes, Stellar Luminosity, Stellar Magnitude, Stellar Orbits

Scientific paper

Five-color light curves have been obtained for the radiation of N Her 1934 which embrace practically the whole orbital cycle of the system. The observations were carried out with a time resolution of 25-45 sec on the 1.25-m AZT-11 telescope at the Crimean Astrophysical Observatory, in five broad-band filters close to the standard UBVRI bands. Results suggest that now approximately 50 years after the 1934 outburst of the nova, the conditions for the development of the next stage in its activity may have arisen.

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