From the 1 of 2.6k papers with an AI index.
10.9k citations
- Centre National de la Recherche ScientifiqueFR904 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR750 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR740 papers
- CEA Paris-SaclayFR725 papers
- Fermi National Accelerator LaboratoryUS675 papers
- European Organization for Nuclear ResearchCH670 papers
- Joint Institute for Nuclear ResearchRU643 papers
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ631 papers
- Institute for High Energy PhysicsES622 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT621 papers
- National and Kapodistrian University of AthensGR621 papers
- Rutherford Appleton LaboratoryGB612 papers
7 papers · 2 filters
On the origin of the Schechter-like mass function of young star clusters in disk galaxies
Patrick Lieberz, Pavel Kroupa
The mass function of freshly formed star clusters is empirically often described as a power law. However the cluster mass function of populations of young clusters over the scale o…
The bound fraction of young star clusters
N. Brinkmann, S. Banerjee, B. Motwani +1
The residual gas within newly formed star clusters is expelled through stellar feedback on timescales ~ 1 Myr. The subsequent expansion of the cluster results in an unbinding of a…
Anisotropy in the all-sky distribution of galaxy morphological types
Behnam Javanmardi, Pavel Kroupa
We present the first study of the isotropy of the distribution of morphological types of galaxies in the Local Universe out to around 200 Mpc using more than 60,000 galaxies from t…
Star formation triggered by galaxy interactions in modified gravity
Florent Renaud, Benoit Famaey, Pavel Kroupa
Together with interstellar turbulence, gravitation is one key player in star formation. It acts both at galactic scales in the assembly of gas into dense clouds, and inside those s…
Hypervelocity stars from young stellar clusters in the Galactic Centre
Giacomo Fragione, Roberto Capuzzo-Dolcetta, Pavel Kroupa
The enormous velocities of the so called hypervelocity stars (HVSs) derive, likely, from close interactions with massive black holes, binary stars encounters or supernova explosion…
Understanding the internal dynamics of elliptical galaxies without non-baryonic dark matter
J. Dabringhausen, P. Kroupa, B. Famaey +1
Assuming virial equilibrium and Newtonian dynamics, low-mass early-type galaxies have larger velocity dispersions than expected from the amount of baryons they contain. The convent…