activity
20092019
most citedMulti-band optical variability of the Blazar S5 0716+714 in outburst state during 2014-2015

44 citations · 111 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2019★ 2 cited

Colours of the flickering source of Mira

R. Zamanov, S. Boeva, B. Spassov +3

We report photometric observations in Johnson UBV bands of the short term variability of Mira. The amplitude detected is 0.16 mag in B band. Adopting interstellar extinction E(B-V)…

astro-ph.SR2018★ 16 cited

The recurrent nova RS Oph - simultaneous B and V band observations of the flickering variability

R. K. Zamanov, S. Boeva, G. Y. Latev +7

We performed 48.6 hours (in 28 nights) of simultaneous B and V band observations of the flickering variability of the recurrent nova RS Oph in quiescence. During the time of our ob…

astro-ph.SR2016★ 2 cited

The cataclysmic variable AE Aquarii: B-V colour of the flares

R. K. Zamanov, G. Y. Latev, S. Boeva +3

We report simultaneous observations of the flaring behaviour of the cataclysmic variable star AE Aqr. The observations are in Johnson B and V bands. The colour-magnitude diagrams (…

astro-ph.SR2015★ 5 cited

Flickering of accreting white dwarfs: the remarkable amplitude-flux relation and disc viscosity

R. K. Zamanov, S. Boeva, G. Latev +7

We analyze optical photometric data of short term variability (flickering) of accreting white dwarfs in cataclysmic variables (KR Aur, MV Lyr, V794 Aql, TT Ari, V425 Cas), recurren…

astro-ph.HE2015★ 44 cited

Multi-band optical variability of the Blazar S5 0716+714 in outburst state during 2014-2015

Aditi Agarwal, Alok C. Gupta, R. Bachev +7

We analyzed the multi-band optical behaviour of the BL Lacertae object, S5 0716+714, during its outburst state from 2014 November - 2015 March. We took data on 23 nights at three o…

astro-ph.SR2015★ 16 cited

Optical Flickering of the recurrent nova RS Ophiuchi: amplitude - flux relation

R. Zamanov, G. Latev, S. Boeva +7

We report observations of the flickering variability of the symbiotic recurrent nova RS~Oph at quiescence in five bands (). We find evidence of a correlation between the pea…