Hostname: page-component-78c5997874-s2hrs Total loading time: 0 Render date: 2024-11-14T08:43:39.272Z Has data issue: false hasContentIssue false

Multiwavelength Variability in the Symbiotic Nova V1016 CYG

Published online by Cambridge University Press:  22 February 2018

Š. Parimucha
Affiliation:
Institute of Physics, Faculty of Natural Sciences, University of P. J. Šafárik, Moyzesova 16 04001 Košice, The Slovak Republic (parmuch@ta3.sk)
M. Vańko
Affiliation:
Astr. Institute of the Slovak Academy of Sciences, 05960 Tatranská Lomnica, The Slovak Republic (vanko@ta3.sk)

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Analysis of the optical and infrared photometry together with UV spectroscopy led to discovery of the 15-years periodicity in the symbiotic system V1016 Cyg. This period could be interpreted as a orbital period in the binary system consisting of the Mira variable and the hot white dwarf.

We have analyzed long-term optical photographic and UBV photoelectric photometry of V1016 Cyg. Collected observations cover pre- and post-outburst stages of the system. The light, curve suggests four stages of activity: the pre-out burst flare in 1949, the main nova-like outburst in 1904, and two post-outbursts, decreasing-amplitude flares in 1980 and 1994, respectively. Activity episodes affecting the system repeat with an interval of ~ 15 years. The ephemeris for the activity maxima is (see Parimucha et al., 2000).

Type
The Contributed Papers
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Nussbaumer, H., & Schild, H. 1981. A&A, 101, 118 Google Scholar
Parimucha, Š., Arkhipova, V. P., Chochol, D., et al., 2000. CAOSP, 30, 99 Google Scholar
Parimucha, Š. 2003, CAOSP 33, 99 Google Scholar
Taranova, O. G., & Yudin, B. F. 1986, AZh. 63, 317 Google Scholar
Whitelock, P. A. 1987. PASP. 99, 573 Google Scholar