10.9k citations
- Centre National de la Recherche ScientifiqueFR2.4k papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR1.9k papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR1.9k papers
- Czech Technical University in PragueCZ1.8k papers
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ1.8k papers
- European Organization for Nuclear ResearchCH1.7k papers
- Heidelberg UniversityDE1.7k papers
- The University of TokyoJP1.7k papers
- University of CopenhagenDK1.7k papers
- University of BirminghamGB1.6k papers
- University of TsukubaJP1.6k papers
- University of LiverpoolGB1.6k papers
28 papers · 2 filters
Characterizing epochs of star formation across the Milky Way disc using age-metallicity distributions of GALAH stars
Christian L. Sahlholdt, Sofia Feltzing, Diane K. Feuillet
We provide a detailed map of the ages and metallicities of turnoff stars in the Milky Way disc based on data from GALAH DR3 and Gaia EDR3. From this map, we identify previously und…
EDGE: What shapes the relationship between HI and stellar observables in faint dwarf galaxies?
Martin P. Rey, Andrew Pontzen, Oscar Agertz +5
We show how the interplay between feedback and mass-growth histories introduces scatter in the relationship between stellar and neutral gas properties of field faint dwarf galaxies…
Gaia-ESO Survey: Detailed elemental abundances in red giants of the peculiar globular cluster NGC 1851
G. Tautvaisiene, A. Drazdauskas, A. Bragaglia +24
Context. NGC 1851 is one of several globular clusters for which multiple stellar populations of the subgiant branch have been clearly identified and a difference in metallicity det…
Self-consistent modelling of the Milky Way's Nuclear Stellar Disc
Mattia C. Sormani, Jason L. Sanders, Tobias K. Fritz +14
The Nuclear Stellar Disc (NSD) is a flattened high-density stellar structure that dominates the gravitational field of the Milky Way at Galactocentric radius $30\lesssim R\lesssim…
From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
Timmy Ejdetjärn, Oscar Agertz, Göran Östlin +2
Supersonic gas turbulence is a ubiquitous property of the interstellar medium. The level of turbulence, quantified by the gas velocity dispersion (), is observed to incr…
MOCCA-SURVEY Database II -- Properties of Intermediate Mass Black Holes escaping from star clusters
Konrad Maliszewski, Mirek Giersz, Dorota Gondek-Rosińska +2
In this work we investigate properties of intermediate-mass black holes (IMBHs) that escape from star clusters due to dynamical interactions. The studied models were simulated as p…