5.1k citations
- Centre National de la Recherche ScientifiqueFR316 papers
- Canadian Institute for Advanced ResearchCA283 papers
- Perimeter InstituteCA230 papers
- University of TorontoCA213 papers
- European Southern ObservatoryCL179 papers
- University of WaterlooCA165 papers
- University of WashingtonUS160 papers
- Max Planck Institute for AstronomyDE154 papers
- Center for Astrophysics Harvard & SmithsonianUS148 papers
- University of CambridgeGB147 papers
- Brockhouse Institute for Materials ResearchCA140 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR135 papers
31 papers · 2 filters
Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +11
The mode of star formation that results in the formation of globular clusters and young massive clusters is difficult to constrain through observations. We present models of massiv…
The PHANGS-AstroSat Atlas of Nearby Star Forming Galaxies
Hamid Hassani, Erik Rosolowsky, Eric W. Koch +29
We present the Physics at High Angular resolution in Nearby GalaxieS (PHANGS)-AstroSat atlas, which contains ultraviolet imaging of 31 nearby star-forming galaxies captured by the…
Testing the Surface Brightness Fluctuation Method on Dwarf Galaxies in the COSMOS Field
Lauren M. Foster, James E. Taylor, John P. Blakeslee
Dwarf galaxies are important tracers of small-scale cosmological structure, yet much of our knowledge about these systems comes from the limited sample of dwarf galaxies within the…
Spectral reconstruction for radiation hydrodynamic simulations of galaxy evolution
Bernhard Baumschlager, Sijing Shen, James W. Wadsley
Radiation from stars and AGN plays an important role in galaxy formation and evolution, and profoundly transforms the IGM, CGM & ISM. On-the-fly RT has started being incorporated i…
A sensitive, high-resolution, wide-field IRAM NOEMA CO(1-0) survey of the very nearby spiral galaxy IC 342
M. Querejeta, J. Pety, A. Schruba +31
We present a new wide-field 10.75 x 10.75 arcmin^2 (~11x11 kpc^2), high-resolution (theta = 3.6" ~ 60 pc) NOEMA CO(1-0) survey of the very nearby (d=3.45 Mpc) spiral galaxy IC 342.…
Galactic properties that favour star cluster formation: a statistical view
Samantha C. Berek, Marta Reina-Campos, Gwendolyn Eadie +1
The presence or absence of star clusters in galaxies, and the properties of star cluster populations compared to their host galaxy properties, are important observables for validat…