446 citations
- Ludwig-Maximilians-Universität MünchenDE61 papers
- Max Planck Institute for Extraterrestrial PhysicsDE26 papers
- Centre National de la Recherche ScientifiqueFR19 papers
- Trieste Astronomical ObservatoryIT16 papers
- University of Hawaii SystemUS14 papers
- Max Planck Institute for AstrophysicsDE13 papers
- Université Bourgogne Franche-ComtéFR11 papers
- Max Planck Institute for AstronomyDE10 papers
- University of CambridgeGB10 papers
- Space Telescope Science InstituteUS9 papers
- University of MichiganUS9 papers
- Excellence Cluster UniverseDE8 papers
73 papers
A ~600 pc view of the strongly-lensed, massive main sequence galaxy J0901: a baryon-dominated, thick turbulent rotating disk with a clumpy cold gas ring at z = 2.259
Daizhong Liu, N. M. Förster Schreiber, R. Genzel +19
We present a high-resolution kinematic study of the massive main-sequence star-forming galaxy (SFG) SDSS J090122.37+181432.3 (J0901) at z=2.259, using 0.36 arcsec ALMA CO(3-2) and…
The metallicity and distance of NGC 2403 from blue supergiants
Fabio Bresolin, Rolf-Peter Kudritzki, Miguel A. Urbaneja
We present the first quantitative spectral analysis of blue supergiant stars in the nearby galaxy NGC 2403. Out of a sample of 47 targets observed with the LRIS spectrograph at the…
CHEX-MATE: Morphological analysis of the sample
Maria Giulia Campitiello, Stefano Ettori, Lorenzo Lovisari +17
In this work, we performed an analysis of the X-ray morphology of the 118 CHEX-MATE (Cluster HEritage project with XMM-Newton - Mass Assembly and Thermodynamics at the Endpoint of…
An Interferometric View of H-MM1. I. Direct Observation of NH3 Depletion
Jaime E. Pineda, Jorma Harju, Paola Caselli +14
Spectral lines of ammonia, NH, are useful probes of the physical conditions in dense molecular cloud cores. In addition to advantages in spectroscopy, ammonia has also been sug…
Exploring the role of cosmological shock waves in the Dianoga simulations of galaxy clusters
Susana Planelles, Stefano Borgani, Vicent Quilis +6
Cosmological shock waves are ubiquitous to cosmic structure formation and evolution. As a consequence, they play a major role in the energy distribution and thermalization of the i…
On the small scale turbulent dynamo in the intracluster medium: A comparison to dynamo theory
Ulrich P. Steinwandel, Ludwig M. Boess, Klaus Dolag +1
We present non-radiative, cosmological zoom-simulations of galaxy cluster formation with magnetic fields and (anisotropic) thermal conduction of one very massive galaxy cluster wit…