Half a Century after the Outburst of the Symbiotic Nova V1016 Cyg

Half a Century after the Outburst of the Symbiotic Nova V1016 Cyg

We present the results of our long-term UBV JHKLM photometry and spectroscopic monitoring of the symbiotic nova V1016 Cyg. After its outburst in 1964, the star showed fading in the U, B, V bands at a rate of about 0.03 mag per year. The behavior of the B − V and U − B color indices reflects variatio...

Full description

Bibliographic Details
Main Authors: Arkhipova V. P., Taranova O. G., Ikonnikova N. P., Esipov V. F., Komissarova G. V., Shenavrin V. I.
Format: Article
Language:English
Published: De Gruyter 2016-03-01
Series:Open Astronomy
Subjects:
binaries: symbiotic
stars: variables: miras
stars: individual (v1016 cyg)
Online Access:https://doi.org/10.1515/astro-2017-0107

Internet

https://doi.org/10.1515/astro-2017-0107

Similar Items