1. The symbiotic binary <scp>ZZ CMi</scp> : Intranight variability and suggested outbursting nature
- Author
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N. A. Tomov, Josep Martí, R. K. Zamanov, Grigor Nikolov, K. A. Stoyanov, Georgi Latev, Svetlana Boeva, Michael F. Bode, Pedro L. Luque-Escamilla, Alexander Kurtenkov, Andon Kostov, and Y. M. Nikolov
- Subjects
Physics ,Accretion (meteorology) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Binary number ,White dwarf ,Astronomy and Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,B band ,Stars ,Amplitude ,Astrophysics - Solar and Stellar Astrophysics ,Space and Planetary Science ,Symbiotic star ,Astrophysics::Solar and Stellar Astrophysics ,Astrophysics::Earth and Planetary Astrophysics ,Emission spectrum ,Astrophysics::Galaxy Astrophysics ,QC ,Solar and Stellar Astrophysics (astro-ph.SR) ,QB - Abstract
We present photometric and spectral observations of the symbiotic star ZZ CMi. We detect intranight variability - flickering and smooth variations in U band. The amplitude of the flickering is about 0.10-0.20 mag in U band. In the B band the variability is lower, with amplitude less than 0.03 mag. We also detect variability in the H-alpha and H-beta emission lines, and find an indication for outflow with velocity of about 120-150 km/s. The results indicate that ZZ CMi is an accretion powered symbiotic containing an M4-M6 III cool component with an white dwarf resembling recurrent novae and jet-ejecting symbiotic stars. [The data are available on www.astro.bas.bg/~rz/ZZCMi/ZZCMi.tar.gz], Comment: accepted in Astronomische Nachrichten / Astronomical Notes
- Published
- 2021