- University of WaterlooCA2.3k papers
- Centre National de la Recherche ScientifiqueFR704 papers
- California Institute of TechnologyUS546 papers
- University of TorontoCA486 papers
- University of CambridgeGB475 papers
- Massachusetts Institute of TechnologyUS433 papers
- University College LondonGB425 papers
- Canadian Institute for Theoretical AstrophysicsCA401 papers
- University of OxfordGB357 papers
- Princeton UniversityUS353 papers
- Sorbonne UniversitéFR342 papers
- Harvard UniversityUS326 papers
11 papers · 2 filters
ALMA observations of massive molecular gas filaments encasing radio bubbles in the Phoenix cluster
H. R. Russell, M. McDonald, B. R. McNamara +11
We report new ALMA observations of the CO(3-2) line emission from the molecular gas reservoir in the central galaxy of the Phoenix c…
Unique probe of dark matter in the core of M87 with the Event Horizon Telescope
Thomas Lacroix, Mansour Karami, Avery E. Broderick +2
We demonstrate the unprecedented capabilities of the Event Horizon Telescope (EHT) to image the innermost dark matter profile in the vicinity of the supermassive black hole at the…
Mass Distribution in Galaxy Cluster Cores
M. T. Hogan, B. R. McNamara, F. Pulido +5
Many processes within galaxy clusters, such as those believed to govern the onset of thermally unstable cooling and AGN feedback, are dependent upon local dynamical timescales. How…
MiNDSTEp differential photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756: Microlensing and a new time delay
E. Giannini, R. W. Schmidt, J. Wambsganß +52
We present V and R photometry of the gravitationally lensed quasars WFI2033-4723 and HE0047-1756. The data were taken by the MiNDSTEp collaboration with the 1.54 m Danish telescope…
Molecular Gas Along a Bright H-alpha Filament in 2A 0335+096 Revealed by ALMA
A. N. Vantyghem, B. R. McNamara, H. R. Russell +17
We present ALMA CO(1-0) and CO(3-2) observations of the brightest cluster galaxy (BCG) in the 2A 0335+096 galaxy cluster (z = 0.0346). The total molecular gas mass of (1.13+/-0.15)…
Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
Kyle A. Oman, Michael J. Hudson
We measure the star formation quenching efficiency and timescale in cluster environments. Our method uses N-body simulations to estimate the probability distribution of possible or…