From the 1 of 30 papers with an AI index.
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- Center for Astrophysics Harvard & SmithsonianUS4 papers
- New Mexico State UniversityUS3 papers
- Agenzia Spaziale ItalianaIT2 papers
- Centre National de la Recherche ScientifiqueFR2 papers
- Český metrologický institutCZ2 papers
- Czech Academy of Sciences, Astronomical InstituteCZ2 papers
- European Southern ObservatoryCL2 papers
- Fondazione Bruno KesslerIT2 papers
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ2 papers
- Graz University of TechnologyAT2 papers
- Heidelberg UniversityDE2 papers
- Istituto Nazionale di Fisica NucleareIT2 papers
4 papers · 1 filter
Powerful Radio Sources in the Southern Sky. IV. Observations of the G4Jy-3CRE Catalog with the Australian Square Kilometre Array Pathfinder
Siegfried A. Gawenda, Juan P. Madrid, Francesco Massaro +19
A recent 2023 paper by Massaro et al. introduced the G4Jy-3CRE, a new catalog of the brightest radio sources in the southern hemisphere that serve as a southern equivalent to the T…
Eclipses of Nearby Millimeter-Bright Galactic Nuclei by Stars in Nuclear Star Clusters
Michal ZajaÄek, Michal Zajaček
It is of a general interest to look for signatures of stellar bodies orbiting supermassive black holes (SMBHs) in galactic nuclei other than the Galactic center. Previously stellar…
The splash beneath the largest radio bubble in a cluster core
H. R. Russell, P. E. J. Nulsen, A. C. Fabian +3
We present a 100 ks XRISM Resolve observation of the Ophiuchus cluster that measures turbulence and bulk motion in the wake of the largest radio bubble on the sky. We detect a sign…
HST view of NGC 5044: Constraints on Filament Widths, Magnetic Support, Multiphase Structure, and Comparison with Cluster Environments
Prathamesh Tamhane, Ming Sun, William Waldron +12
We present new Hubble Space Telescope (HST) imaging of ionised filaments in the brightest group galaxy NGC 5044. These filaments extend several kiloparsecs and have widths of $\sim…