Intrinsic and Environmental Effects on the Distribution of Star Formation in TNG100 Galaxies
We present radial profiles of luminosity-weighted age (age _L ) and ΔΣ _SFR for various populations of high- and low-mass central and satellite galaxies in the TNG100 cosmological simulation.
Bryanne McDonough +2 more
doaj +1 more source
A TALE OF TWO FEEDBACKS: STAR FORMATION IN THE HOST GALAXIES OF RADIO AGNs [PDF]
Marios Karouzos +21 more
openalex +1 more source
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source
The relationship between obscured AGN and their host galaxies
This thesis presents an investigation into obscured Active Galactic Nuclei (AGN) activity at high redshift and the interactions they share with their host galaxies. Using a combination of X-ray spectral fitting and X-ray stacking analyses, three studies are undertaken in this work.
openaire +4 more sources
Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S +7 more
europepmc +1 more source
Ionized outflows in luminous type 2 AGNs atz< 0.6: no evidence for significant impact on the host galaxies [PDF]
M. Villar‐Martín +7 more
openalex +1 more source
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning. [PDF]
Kugel R +19 more
europepmc +1 more source
We present detailed and comprehensive data reduction and point-spread-function (PSF) model construction for all public JWST NIRCam imaging data from the COSMOS-Web treasury program (up to 2023 June, totaling 0.28 deg ^2 ). We show that the NIRCam PSF has
Ming-Yang Zhuang, Junyao Li, Yue Shen
doaj +1 more source
The environments of the radio galaxy population in simba. [PDF]
Thomas N, Davé R.
europepmc +1 more source
Narrow [O iii] Emission Lines as a Potential Proxy for the Evolutionary Stage of Quasars
Radio spectral shape of quasars can provide insight into the ages of quasars. We have compiled data for 1804 quasars with z ≲ 1 from the Sloan Digital Sky Survey (SDSS).
Zhi-fu Chen +3 more
doaj +1 more source

