output
20022026
most citedThe ACS Nearby Galaxy Survey Treasury

564 citations

Showing 2019 · astro-ph.GAShow all

8 papers · 2 filters

astro-ph.GA20194 cited

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…

astro-ph.GA20192 cited

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…

astro-ph.GA20198 cited

Properties of galaxies with an offset between the position angles of the major kinematic and photometric axes

L. S. Pilyugin, E. K. Grebel, I. A. Zinchenko +4

We derive the photometric, kinematic, and abundance characteristics of 18 star-forming MaNGA galaxies with fairly regular velocity fields and surface brightness distributions and w…

astro-ph.GA20195 cited

Globular Cluster Systems and X-Ray Atmospheres in Galaxies

Gretchen L. H. Harris, Iurii V. Babyk, William E. Harris +1

We compare the empirical relationships between the mass of a galaxy's globular system M_GCS, the gas mass in the hot X-ray atmosphere M_X within a fiducial radius of 5 r_e, the tot…

astro-ph.GA20198 cited

'Scraggy' dark halos around bulge-less spiral galaxies

I. D. Karachentsev, V. E. Karachentseva

We use a sample of 220 face-on bulge-less galaxies situated in the low density environment to estimate their total mass via orbital motions of supposed rare satellites. Our inspect…

astro-ph.GA201917 cited

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…