activity
20152026
most citedGaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy

81 citations · 243 across the 23 of their papers we have counts for

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13 papers · 1 filter

astro-ph.SR2026

Is Mira B a low mass white dwarf?

R. K. Zamanov, V. Irincheva, B. Spassov +8

We report photometric observations in Johnson B and V bands of the short term variability (flickering) of Mira (omicron Ceti). The observations were performed during 7 nights in th…

astro-ph.SR2024★ 3 cited

Evolution of the optical emission lines and the X-ray emission during the super-active stage of T CrB

K. A. Stoyanov, G. J. M. Luna, R. K. Zamanov +6

T CrB is a symbiotic star that experiences nova outbursts every 80~yr. The next, long-anticipated nova outburst should occur during the 2024-2026 period. Here, we present re…

astro-ph.SR2022★ 1 cited

The hidden symbiotic star SU Lyn -- detection of flickering in U band

R. K. Zamanov, A. Kostov, M. Moyseev +18

We report photometric observations of the hidden symbiotic star SU Lyn in the optical bands. In five nights we detect a weak flickering in U band with amplitude of about 0.05 magni…

astro-ph.SR2022★ 1 cited

A Long-Term Spectral Study of the Single Active Giant OP Andromedae

Stefan Georgiev, Renada Konstantinova-Antova, Ana Borisova +10

We present a spectral study of the single magnetically active K giant OP And in the period 1979 -- 2018, monitoring the variability of the activity indicator line H. Original da…

astro-ph.SR2022

Ultra-short period contact binaries: restricting the parameters of the primary using Gaia parallax

Alexander Kurtenkov

Possible M-type contact binaries were investigated by selecting W UMa-type variables with orbital periods below the 0.22-day cutoff. Gaia parallaxes were combined with Gaia and 2MA…

astro-ph.SR2022★ 12 cited

The origin of the high-mass X-ray binary 4U 2206+54/BD +53 2790

V. Hambaryan, K. A. Stoyanov, M. Mugrauer +7

Based on the Gaia EDR3 astrometric parameters and our new systemic radial velocity of the high-mass X-ray binary 4U 2206+54/BD+53 2790, we studied the trace back motion of the syst…

astro-ph.SR2021★ 6 cited

The symbiotic binary ZZ CMi: intranight variability and suggested outbursting nature

R. K. Zamanov, K. A. Stoyanov, A. Kostov +9

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 f…

astro-ph.SR2020★ 3 cited

Flickering of the jet-ejecting symbiotic star MWC 560

R. K. Zamanov, S. Boeva, K. A. Stoyanov +4

We analyse optical photometric data of short term variability (flickering) of the accreting white dwarf in the jet-ejecting symbiotic star MWC560. The observations are obtained in…

astro-ph.SR2019

The observed temperature distribution of contact binaries derived from SDSS photometry

Alexander Kurtenkov, Mirela Napetova

Data from the VSX, SDSS DR12, and Gaia DR2 catalogs were combined in order to explore the observed temperature distribution of known contact binaries. Color-temperature relations w…

astro-ph.SR2017

Optical flickering of the symbiotic star CH Cyg

K. A. Stoyanov, J. Marti, R. Zamanov +6

Here we present quasi-simultaneous observations of the flickering of the symbiotic binary star CH Cyg in U, B and V bands. We calculate the flickering source parameters and discuss…

astro-ph.SR2016

Searching for twins of the V1309 Sco progenitor system: a selection of long-period contact binaries

Alexander Kurtenkov

The only well-studied red nova progenitor (V1309 Sco) was a contact binary with a 1.4-day period. The prospects for searching for similar systems, as well as stellar merger candida…

astro-ph.SR2016★ 2 cited

Improved proper motion determinations for 15 open clusters based on the UCAC4 catalog

Alexander Kurtenkov, Nadezhda Dimitrova, Alexander Atanasov +1

The proper motions of 15 nearby (d < 1 kpc) open clusters were recalculated using data from the UCAC4 catalog. Only evolved or main sequence stars inside a certain radius from the…

astro-ph.SR2015★ 36 cited

The January 2015 outburst of a red nova in M31

Alexander Kurtenkov, Peter Pessev, Toma Tomov +19

M31N 2015-01a (or M31LRN 2015) is a red nova that erupted in January 2015 -- the first event of this kind observed in M31 since 1988. Very few similar events have been confirmed as…