112 citations · 279 across the 6 of their papers we have counts for
8 papers
Do the majority of stars form as gravitationally unbound?
František Dinnbier, Pavel Kroupa, Richard I. Anderson
Some of the youngest stars (age Myr) are clustered, while many others are observed scattered throughout star forming regions or in complete isolation. It has been int…
Tree-based solvers for adaptive mesh refinement code FLASH -- II: radiation transport module TreeRay
Richard Wünsch, Stefanie Walch, František Dinnbier +5
The treatment of radiative transfer with multiple radiation sources is a critical challenge in simulations of star formation and the interstellar medium. In this paper we present t…
SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
Tim-Eric Rathjen, Thorsten Naab, Philipp Girichidis +6
We present simulations of the multi-phase interstellar medium (ISM) at solar neighbourhood conditions including thermal and non-thermal ISM processes, star cluster formation, and f…
How fast do young star clusters expel their natal gas?: Estimating the upper limit of the gas expulsion time-scale
F. Dinnbier, S. Walch
Formation of massive stars within embedded star clusters starts a complex interplay between their feedback, inflowing gas and stellar dynamics, which often includes close stellar e…
Tidal tails of open star clusters as probes to early gas expulsion II: Predictions for Gaia
František Dinnbier, Pavel Kroupa
We study the formation and evolution of the tidal tail released from a young Pleiades-like star cluster, due to expulsion of primordial gas in a realistic gravitational field of th…
Tidal tails of open star clusters as probes to early gas expulsion I: A semi-analytic model
František Dinnbier, Pavel Kroupa
Star clusters form out of the densest parts of infrared dark clouds. The emergence of massive stars expels the residual gas, which has not formed stars yet. Gas expulsion lowers th…