35 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Instituto de Astrofísica de CanariasES6 papers
- Universidad de La LagunaES6 papers
- European Southern ObservatoryCL5 papers
- Adler PlanetariumUS4 papers
- Astronomy and SpaceAU4 papers
- Centre National de la Recherche ScientifiqueFR4 papers
- Charles UniversityCZ4 papers
- Consejo Superior de Investigaciones CientíficasES4 papers
- Fundação Planetário da Cidade do Rio de JaneiroBR4 papers
- Institute of Astrophysics and Space SciencesPT4 papers
- McGill UniversityCA4 papers
- McMaster UniversityCA4 papers
6 papers · 1 filter
Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies
C. Marrero-de la Rosa, J. Méndez-Abreu, A. de Lorenzo-Cáceres +20
In the standard cold dark matter (CDM) cosmology, the existence of massive pure-disc galaxies remains challenging within the hierarchical framework and is key to understandi…
Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
Salvador Cardona-Barrero, Jairo Méndez-Abreu, Adriana de Lorenzo-Cáceres +17
. The existence of massive disc galaxies with little or no bulge challenges conventional cold dark matter model, which typically favours dynamically hot central structure…
Primordial mass segregation of star clusters: The role of binary stars
Václav Pavlík
Observational results of young star-forming regions suggest that star clusters are completely mass segregated at birth. As a star cluster evolves dynamically, these initial conditi…
The hunt for self-similar core collapse
Václav Pavlík, Ladislav Šubr
Core collapse is a prominent evolutionary stage of self-gravitating systems. In an idealised collisionless approximation, the region around the cluster core evolves in a self-simil…
The black hole retention fraction in star clusters
Václav Pavlík, Tereza Jeřábková, Pavel Kroupa +1
Recent research has been constraining the retention fraction of black holes (BHs) in globular clusters by comparing the degree of mass segregation with -body simulations. They a…
Neutron stars and millisecond pulsars in star clusters: implications for the diffuse -radiation from the Galactic Centre
Giacomo Fragione, Václav Pavlík, Sambaran Banerjee
Globular clusters (GCs) are the ideal environment for the formation of neutron stars (NSs) and millisecond pulsars (MSPs). NSs origin and evolution provide a useful information on…