activity
20082026
most citedThe awakening of BL Lacertae: observations by Fermi, Swift, and the GASP-WEBT

135 citations · 536 across the 55 of their papers we have counts for

collaborators

55 papers

astro-ph.SR2026

H_alpha observations of the Be/X-ray binary MWC 656

R. Zamanov, V. Marchev, K. A. Stoyanov +8

Context. MWC 656 is a Be/X-ray binary identified as an emission-line object, X-ray and radio source and might be a weak gamma-ray source, harbouring an enigmatic secondary componen…

astro-ph.SR2025

Red giant component of the recurrent nova T Coronae Borealis

R. K. Zamanov, D. Marchev, V. Marchev +5

We performed simultaneous V band photometry and spectroscopic observations of the recurrent nova T CrB and estimate the V band magnitude of the red giant. We find for the red giant…

astro-ph.SR2025

Interstellar extinction toward MWC 148

R. Zamanov, I. Stateva, J. Marti +2

We analyse high resolution optical spectra of MWC148 (optical counterpart of the gamma-ray source HESS J0632+057) obtained at Observatoire de Haute Provence and Rozhen Observatory.…

astro-ph.SR2024★ 10 cited

Investigation of the Nature of the B[e] Star CI Cam in the Optical Range

E. A. Barsukova, A. N. Burenkov, V. P. Goranskij +10

We report the results of 24 years of photometric and spectroscopic monitoring of CI Cam since its outburst in 1998. In the early years of our research, we identified a system compo…

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.SR2024★ 1 cited

Size of the accretion disc in the recurrent nova T CrB

R. K. Zamanov, K. A. Stoyanov, V. Marchev +7

We present high resolution (0.06 A/px) spectroscopic observations of the recurrent nova T Coronae Borealis obtained during the last 1.5 years (September 2022 -- January 2024), with…

astro-ph.SR2024

Luminosity class of the symbiotic stars 4U1954+319 and ZZ CMi

R. Zamanov, K. A. Stoyanov, G. Latev +8

We performed optical photometry and spectral observations of the symbiotic stars 4U1954+319 and ZZ CMi. For 4U1954+319 using high-resolution spectra we measure the equivalent width…

astro-ph.SR2023★ 17 cited

Symbiotic star T CrB as an extreme SU UMa type dwarf nova

Krystian Ilkiewicz, Joanna Mikolajewska, Kiril A. Stoyanov

T CrB is a symbiotic recurrent nova that exhibits quiescent and active phases between its classical nova eruptions. The statistical properties of these active phases have been poor…

astro-ph.SR2023

BV photometric observations of the flickering of the dwarf nova RX And

R. K. Zamanov, L. Dankova, M. Moyseev +3

We report photometry of the intranight variability of the dwarf nova RX And in two bands (B and V). The observations are carried out during three nights in November-December 2022 a…

astro-ph.SR2023★ 4 cited

Optical spectroscopy of Be stars: peak separation of Balmer emission lines

R. K. Zamanov, K. A. Stoyanov, S. Y. Stefanov +2

The Be stars display variable optical emission lines originating in the circumstellar disc. Here we analyse high resolution spectroscopic observations of Be stars and the distance…

astro-ph.SR2023★ 4 cited

Mass outflow from the symbiotic binary RS Oph during its 2021 outburst

N. A. Tomov, M. T. Tomova, K. A. Stoyanov +7

RS Oph is a symbiotic recurrent nova containing a massive white dwarf with heavy mass loss during activity. In August 2021, it underwent its seventh optical eruption since the end…

astro-ph.SR2022★ 1 cited

For optical flickering in symbiotic star MWC 560

Dragomir Marchev, Kiril Stoyanov, Vladislav Marchev +5

This study is based on observations of MWC560 during the last two observational seasons (2020/2021 and 2021/2022). Other than looking for flickering we were interested in following…

astro-ph.SR2022★ 6 cited

Optical spectroscopy of the Be/black hole binary MWC656 -- interaction of a black hole with a circumstellar disc

R. K. Zamanov, K. A. Stoyanov, D. Marchev +7

We present new spectroscopic observations of the Be/black hole binary MWC 656 obtained during the period 2015 - 2021. We measure the equivalent width of H (EW), H (…

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★ 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★ 16 cited

SU Lyn -- a transient symbiotic star

Krystian Ilkiewicz, Joanna Mikolajewska, Simone Scaringi +3

SU Lyn is a binary system composed of a white dwarf and a red giant star. Although it is known to be bright and variable at X-ray wavelengths, the optical counterpart of the source…

astro-ph.SR2021★ 3 cited

H-alpha spectroscopy of the recurrent nova RS Oph during the 2021 outburst

R. K. Zamanov, K. A. Stoyanov, Y. M. Nikolov +3

We report spectroscopic observations of the emission line of the recurrent nova RS~Oph obtained between 12 and 23 August 2021 during the recent outburst. On the basis of the s…

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

Interstellar extinction toward symbiotic stars

R. K. Zamanov, V. D. Marchev, K. A. Stoyanov

Using diffuse interstellar bands (DIBs) at 5780 A, 5797 A and 6613 A, visible in the high resolution spectra, and measuring their equivalent widths, we estimate the interstellar ex…

astro-ph.SR2020★ 3 cited

Optical spectroscopy and X-ray observations of the D-type symbiotic star EF Aql

K. A. Stoyanov, K. Iłkiewicz, G. J. M. Luna +6

We performed high-resolution optical spectroscopy and X-ray observations of the recently identified Mira-type symbiotic star EF Aql. Based on high-resolution optical spectroscopy o…

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.SR2020

Intra-night flickering of RS Ophiuchi: III. Modes of quasi-periods in the minute scale and their evolution

Ts. B. Georgiev, R. K. Zamanov, S. Boeva +7

We study the photometric behavior of the recurrent nova RS Oph by 58 monitoring light curves (LCs), taken by 5 telescopes. All LCs show repeating time structures with some quasi-pe…

astro-ph.SR2019

High-resolution optical spectroscopy of Nova V392 Per

K. A. Stoyanov, T. Tomov, I. Stateva +1

Here we analyze high-resolution spectra of the Nova V392 Per obtained during the 2018 outburst. The H and H emission lines show a triple-peak structure with radial velocities…

astro-ph.SR2019★ 2 cited

An eccentric wave in the circumstellar disc of the Be/X-ray binary X Persei

R. K. Zamanov, K. A. Stoyanov, U. Wolter +7

We present spectroscopic observations of the Be/X-ray binary X Per obtained during the period December 2017 - January 2020 (MJD~58095 - MJD~58865). In December 2017 the , ,…