140 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Jilin UniversityCN38 papers
- State Key Laboratory of High Pressure and Superhard MaterialsCN13 papers
- National Academy of Sciences of UkraineUA12 papers
- Institute of Radio AstronomyUA9 papers
- Main Astronomical ObservatoryUA6 papers
- Chinese Academy of SciencesCN5 papers
- Heidelberg UniversityDE5 papers
- National Technical University "Kharkiv Polytechnic Institute"UA4 papers
- State Key Laboratory on Integrated OptoelectronicsCN4 papers
- Center for Advanced Systems UnderstandingDE3 papers
- Jilin Medical UniversityCN3 papers
- Lviv UniversityUA3 papers
6 papers · 1 filter
Circumnuclear regions of different BPT types in star-forming MaNGA galaxies: AGN detectability
L. S. Pilyugin, E. K. Grebel, I. A. Zinchenko +3
We consider the circumnuclear regions of MaNGA galaxies. The spectra are classified as AGN-like, HII-region-like (or SF-like), and intermediate (INT) spectra according to their pos…
Simulation of the loss-cone instability in spherical systems. II. Dominating Keplerian potential
E. V. Polyachenko, P. Berczik, A. Just +1
A new so-called `gravitational loss-cone instability' in stellar systems has recently been investigated theoretically in the framework of linear perturbation theory and proved to b…
Simulation of the loss-cone instability in spherical systems. I. Dominating harmonic potential
E. V. Polyachenko, P. Berczik, A. Just +1
A new so-called `gravitational loss-cone instability' in stellar systems has recently been investigated theoretically in the framework of linear perturbation theory and proved to b…
The star cluster survivability after gas expulsion is independent of the impact of the Galactic tidal field
B. Shukirgaliyev, G. Parmentier, P. Berczik +1
We study the impact of the tidal field on the survivability of star clusters following instantaneous gas expulsion. Our model clusters are formed with a centrally-peaked star-forma…
Impact of a star formation efficiency profile on the evolution of open clusters
Bekdaulet Shukirgaliyev, Genevieve Parmentier, Peter Berczik +1
We study the effect of the instantaneous gas expulsion on star clusters wherein the residual gas has a density profile shallower than that of the embedded cluster. This is expected…
Galaxy Rotation and Supermassive Black Hole Binary Evolution
Muhammad Awais Mirza, Afnan Tahir, Fazeel Mahmood Khan +4
Supermassive black hole (SMBH) binaries residing at the core of merging galaxies are recently found to be strongly affected by the rotation of their host galaxies. The highly eccen…