110 citations · 223 across the 7 of their papers we have counts for
7 papers
The masses of open star clusters and their tidal tails and the stellar initial mass function
Henriette Wirth, František Dinnbier, Pavel Kroupa +1
Unresolved binaries have a strong influence on the observed parameters of stellar clusters (SCs). We quantify this influence and compute the resulting mass underestimates and stell…
On the dynamical evolution of Cepheid multiplicity in star clusters and its implications for B-star multiplicity at birth
František Dinnbier, Richard I. Anderson, Pavel Kroupa
Classical Cepheid variable stars provide a unique probe to binary evolution in intermediate-mass stars over the course of several tens to hundreds of Myr. We studied the binary and…
Tree-based solvers for adaptive mesh refinement code FLASH -- III: a novel scheme for radiation pressure on dust and gas and radiative transfer from diffuse sources
A. Klepitko, S. Walch, R. Wünsch +3
Radiation is an important contributor to the energetics of the interstellar medium, yet its transport is difficult to solve numerically. We present a novel approach towards solving…
On the dynamical evolution of Cepheids in star clusters
František Dinnbier, Richard I. Anderson, Pavel Kroupa
We investigate the occurrence of classical (type-I) Cepheid variable stars (henceforth: Cepheids) in dynamically evolving star clusters from birth to an age of approximately 300 My…
The relative impact of photoionizing radiation and stellar winds on different environments
Sebastian Haid, Stefanie Walch, Daniel Seifried +3
Photoionizing radiation and stellar winds from massive stars deposit energy and momentum into the interstellar medium (ISM). They might disperse the local ISM, change its turbulent…
Globular Cluster formation in a collapsing supershell
S. Recchi, R. Wünsch, J. Palous +1
Primordial clouds are supposed to host the so-called population III stars. These stars are very massive and completely metal-free. The final stage of the life of population III sta…
Tree-based solvers for adaptive mesh refinement code FLASH - I: gravity and optical depths
Richard Wünsch, Stefanie Walch, František Dinnbier +1
We describe an OctTree algorithm for the MPI-parallel, adaptive mesh-refinement code {\sc FLASH}, which can be used to calculate the gas self-gravity, and also the angle-averaged l…