collaborators

5 papers

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

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

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

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…