activity
20012023
most citedThe formation of secondary stellar generations in massive young star clusters from rapidly cooling shocked stellar winds

46 citations · 144 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2023★ 1 cited

A 3D model for the stellar populations in the nuclei of NGC 1433,NGC 1566, and NGC 1808

P. Vermot, J. Palouš, B. Barna +3

Aims. We aim to characterize the properties of the stellar populations in the central few hundred parsecs of nearby galactic nuclei; specifically their age, mass, and 3D geometry.…

astro-ph.GA2016★ 46 cited

The formation of secondary stellar generations in massive young star clusters from rapidly cooling shocked stellar winds

Richard Wünsch, Jan Palouš, Guillermo Tenorio-Tagle +1

We study a model of rapidly cooling shocked stellar winds in young massive clusters and estimate the circumstances under which secondary star formation, out of the reinserted winds…

astro-ph.GA2014★ 1 cited

Gould's Belt

Jan Palouš, Soňa Ehlerová

The local velocity patterns of star forming regions, young OB stars, nearby OB associations, atomic and molecular gas are confronted with models of an expanding region. We test fre…

astro-ph.GA2013★ 46 cited

HI shells in the Leiden/Argentina/Bonn HI survey

S. Ehlerova, J. Palous

We analyse the all-sky Leiden/Argentina/Bonn HI survey, where we identify shells belonging to the Milky Way. We used an identification method based on the search of continuous regi…

astro-ph2002★ 41 cited

Environmental Dependencies for Star Formation Triggered by Expanding Shell Collapse

Bruce G. Elmegreen, Jan Palous, Sona Ehlerova

Criteria for gravitational collapse of expanding shells in rotating, shearing galaxy disks were determined using three-dimensional numerical simulations in the thin shell approxima…

astro-ph2001★ 9 cited

The HI supershell GS061+00+51 and its neighbours

S. Ehlerova, J. Palous, W. K. Huchtmeier

We describe HI observations of a 4 x 4 degrees field in the Milky Way centered on l=61 deg, b=0 deg made by the Effelsberg radiotelescope. The field contains one previously identif…