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20012026
most citedAtomic gas far away from the Virgo cluster core galaxy NGC 4388. A possible link to isolated star formation in the Virgo cluster?

47 citations · 183 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Predicting CO and dust emission of star-forming galaxies

B. Vollmer, J. Braine, M. Soida +1

How do Dwarf Galaxies differ from spirals? Does star formation produce radio and far-infrared emission in the same way as in spiral galaxies? Radio, FarIR, and CO emission depend o…

astro-ph.CO2012★ 25 cited

A dynamical model for the Taffy galaxies UGC 12914/5

B. Vollmer, J. Braine, M. Soida

The spectacular head-on collision of the two gas-rich galaxies of the Taffy system, UGC 12914/15, gives us a unique opportunity to study the consequences of a direct ISM-ISM collis…

astro-ph2003★ 47 cited

Atomic gas far away from the Virgo cluster core galaxy NGC 4388. A possible link to isolated star formation in the Virgo cluster?

B. Vollmer, W. Huchtmeier

We have discovered 6 10^7 M_{\odot} of atomic gas at a projected distance greater than 4' (20 kpc) from the highly inclined Virgo spiral galaxy NGC 4388. This gas is most probably…

astro-ph2003★ 35 cited

Turbulent viscosity in clumpy accretion disks II supernova driven turbulence in the Galaxy

B. Vollmer, T. Beckert

An analytical model for a turbulent clumpy gas disk is presented where turbulence is maintained by the energy input due to supernovae. Expressions for the disk parameters, global f…

astro-ph2003★ 40 cited

Magnetic field evolution in galaxies interacting with the intracluster medium. 3D numerical simulations

K. Otmianowska-Mazur, B. Vollmer

A fully three-dimensional (3D) magnetohydrodynamical (MHD) model is applied to simulate the evolution of the large-scale magnetic field in cluster galaxies interacting with the int…

astro-ph2001★ 36 cited

Turbulent viscosity in clumpy accretion disks. Application to the Galaxy

B. Vollmer, T. Beckert

The equilibrium state of a turbulent clumpy gas disk is analytically investigated. The disk consists of distinct self-gravitating clouds. Gravitational cloud-cloud interactions tra…