Наукова електронна бібліотека
періодичних видань НАН України
періодичних видань НАН України
Results of 5-year photometric monitoring of the intermediate polar V2306 Cygni: correction of the orbital period and evidence of 2-day periodicity
Репозиторій DSpace/Manakin
JavaScript is disabled for your browser. Some features of this site may not work without it.
Results of 5-year photometric monitoring of the intermediate polar V2306 Cygni: correction of the orbital period and evidence of 2-day periodicity
Інший ID:
DOI: 10.17721/2227-1481.5.17-20
Посилання:
Results of 5-year photometric monitoring of the intermediate polar V2306 Cygni: correction of the orbital period and evidence of 2-day periodicity / V. Breus, K. Petrík, S. Zoła, A. Baransky, T. Hegedus // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 17-20. — Бібліогр.: 11 назв. — англ.
Підтримка:
We would like to thank William Gof, Etienne Morelle, James Jones, Richard Sabo, J. Ulowetz and the administration of the AAVSO International Database contributed by observers worldwide for the observations used in this research.
Дата:
2015
Переглядів:
839
Завантажень:
472
Анотація:
We present the results of 6 years of photometric monitoring of the magnetic cataclysmic variable V2306 Cygni (formerly known as 1WGA J1958.2+3232) obtained at collaborating observatories. Using (O-C) analysis we tried to study variability of the spin period of the white dwarf, however we cannot make a firm conclusion based on the scatter. Simultaneously, using (O-C) diagram of orbital minima, we found that the value of 0.181545(3) days better corresponds with the light curve, than do previously published orbital period values. We also found that the variability has a 2.01 day period; this variability may be interpreted as possible precession of the accretion disk in this system.
