Results 151 to 160 of about 68,110 (257)

ELUCID. VIII. Simulating the Coma Galaxy Cluster to Calibrate Model and Understand Feedback

The Astrophysical Journal
We conducted an investigation of the Coma cluster of galaxies by running a series of constrained hydrodynamic simulations with GIZMO-SIMBA and GADGET-3 based on initial conditions reconstructed from the SDSS survey volume in the ELUCID project.
Xiong Luo, Huiyuan Wang, Weiguang Cui, Houjun Mo, RenJie Li, Yipeng Jing, Neal Katz, Romeel Davé, Xiaohu Yang, Yangyao Chen, Hao Li, Shuiyao Huang   +11 more
doaj   +1 more source

Are Radio Minihalos Confined by Cold Fronts in Galaxy Clusters? Minihalos and Large-scale Sloshing in A3444 and MS 1455.0+2232

The Astrophysical Journal
We present radio and X-ray studies of A3444 and MS1455.0+2232, two galaxy clusters with radio minihalos in their cool cores. A3444 is imaged using the Giant Metrewave Radio Telescope (GMRT) at 333, 607, and 1300 MHz and the Very Large Array at 1435 MHz ...
S. Giacintucci, T. Venturi, M. Markevitch, G. Brunetti, T. E. Clarke, R. Kale   +5 more
doaj   +1 more source

The Contribution of Population III to the Enrichment and Preheating of the Intracluster Medium [PDF]

, 2001
Michael Loewenstein
openalex   +1 more source

Tracking Dusty Cloud Crushed by a Hot Flow

Universe
The destructionof clouds by strong shocks and hot winds is the key process responsible for the transporting of metals and dust from the ISM to the ICM/IGM, and establishing the multiphase structure in and around galaxies.
Svyatoslav Dedikov, Evgenii Vasiliev
doaj   +1 more source

Forming intracluster gas in a galaxy protocluster at a redshift of 2.16. [PDF]

Nature, 2023
Di Mascolo L, Saro A, Mroczkowski T, Borgani S, Churazov E, Rasia E, Tozzi P, Dannerbauer H, Basu K, Carilli CL, Ginolfi M, Miley G, Nonino M, Pannella M, Pentericci L, Rizzo F.   +15 more
europepmc   +1 more source

On the interaction of FR II radio sources with the intracluster medium [PDF]

, 2002
Paul Alexander
openalex   +1 more source

Chemical Composition of the Intracluster Medium

, 2003
Clusters of galaxies are massive enough to be considered representative samples of the Universe, and to retain all of the heavy elements synthesized in their constituent stars. Since most of these metals reside in hot plasma, X-ray spectroscopy of clusters provides a unique and fundamental tool for studying chemical evolution.
openaire   +2 more sources

Genetic diversity of Ethiopian durum wheat (T. turgidum subsp. durum) landraces under water stressed and non stressed conditions. [PDF]

Heliyon, 2023
Dukamo BH, Gedebo A, Tesfaye B, Degu HD.
europepmc   +1 more source

Star Formation, Nebulae, and Active Galactic Nuclei in CLASH Brightest Cluster Galaxies. I. Dependence on Core Entropy of Intracluster Medium

The Astrophysical Journal
We set the stage for reassessing how star formation, emission-line nebulae, and active galactic nuclei (AGNs) in brightest cluster galaxies (BCGs) depend on the thermodynamics of the intracluster medium (ICM).
Arsen Levitskiy, Jeremy Lim, Youichi Ohyama, Juno Li, Megan Donahue   +4 more
doaj   +1 more source

Magnetic field in the intracluster medium: Rydberg matter with almost free electrons [PDF]

, 2002
Shahriar Badiei, Leif Holmlid
openalex   +1 more source