activity
19992020
most citedA multi-wavelength view on the dusty Wolf-Rayet star WR 48a

209 citations · 709 across the 44 of their papers we have counts for

collaborators

45 papers

astro-ph.SR2020★ 4 cited

A global view on the colliding-wind binary WR 147

Svetozar A. Zhekov, Blagovest V. Petrov, Toma V. Tomov +1

We present results from a global view on the colliding-wind binary WR 147. We analysed new optical spectra of WR 147 obtained with Gran Telescopio CANARIAS and archive spectra from…

astro-ph.SR2020★ 3 cited

International observational campaign of the 2014 eclipse of EE Cep

D. Pieńkowski, C. Gałan, T. Tomov +64

Context. EE Cep is one of few eclipsing binary systems with a dark, dusty disk around an invisible object similar to ε Aur. The system is characterized by grey and asymmetric eclip…

astro-ph.HE2019★ 18 cited

XMM-Newton observations of the symbiotic recurrent nova T CrB: evolution of X-ray emission during the active phase

Svetozar A. Zhekov, Toma V. Tomov

We present an analysis of the XMM-Newton observations of the symbiotic recurrent nova T CrB, obtained during its active phase that started in 2015. The XMM-Newton spectra of T CrB…

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.SR2018★ 2 cited

An XMM-Newton observation of the symbiotic star AG Peg: the X-ray emission after the end of its 2015 outburst

Svetozar A. Zhekov, Toma V. Tomov

We present an analysis of the XMM-Newton observation of the symbiotic star AG Peg, obtained after the end of its 2015 outburst. The X-ray emission of AG Peg is soft and of thermal…

astro-ph.HE2018★ 124 cited

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters

Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…