activity
19982018
most citedAbundance analysis of two late A-type stars HD 32115 and HD 37594

33 citations · 194 across the 15 of their papers we have counts for

collaborators

15 papers

astro-ph.IM2018★ 4 cited

Experimental study of an advanced concept of moderate-resolution holographic spectrographs

Eduard Muslimov, Gennady Valyavin, Sergei Fabrika +4

We present the results of an experimental study of an advanced moderate-resolution spectrograph based on a cascade of narrow-band holographic gratings. The main goal of the project…

astro-ph.IM2016★ 2 cited

ESpeRo: Echelle Spectrograph Rozhen

Tanyu Bonev, Haralambi Markov, Toma Tomov +11

In this paper we describe the echelle spectrograph of the 2 meter telescope of the Rozhen National Astronomical Observatory. The spectrograph is a cross-dispersed, bench-mounted, f…

astro-ph.SR2015★ 19 cited

Spectroscopic variability of IRAS22272+5435

L. Začs, F. Musaev, B. Kaminsky +4

A time series of high-resolution spectra was observed in the optical wavelength region for the bright proto-planetary nebula IRAS22272+5435 (HD235858), along with a simultaneous mo…

astro-ph.GA2015★ 16 cited

The structure and kinematics of the the Galaxy thin gaseous disc outside the solar orbit

G. A. Galazutdinov, A. Strobel, F. A. Musaev +2

The rotation curve of the Galaxy is generally thought to be flat. However, using radial velocities from interstellar molecular clouds, which is common in rotation curve determinati…

astro-ph.SR2012★ 19 cited

International observational campaigns of the last two eclipses in EE Cephei: 2003 and 2008/9

C. Gałan, M. Mikołajewski, T. Tomov +87

Two observational campaigns were carried out during the eclipses of EE Cep in 2003 and 2008/9 to verify whether the eclipsing body in the system is indeed a dark disk and to unders…

astro-ph.SR2011★ 25 cited

The evolutionary status of the UX Orionis star RZ Piscium

V. P. Grinin, I. S. Potravnov, F. A. Musaev

The star RZ Psc is one of the most enigmatic members of the UX Ori star family. It shows all properties that are typical for these stars (the light variability, high linear polariz…