Results 111 to 120 of about 1,770 (180)
The North Polar Spur (NPS) is a prominent diffuse X-ray feature whose origin has remained uncertain for decades. Using a uniform analysis of archival Suzaku and XMM-Newton data with new Chandra observations, we constrain its thermal and chemical ...
Anjali Gupta +7 more
doaj +1 more source
The impact of galactic feedback on the circumgalactic medium
Galactic feedback strongly affects the way galactic environments are enriched. We examine this connection by performing a suite of cosmological hydrodynamic simulations, exploring a range of parameters based on the galaxy formation model developed in ...
Torrey, Paul +7 more
core +1 more source
The Detection Rate of Associated Mg ii Absorption Lines in Quasars Depends on Their Radio Emission
In active galactic nuclei, jet-driven feedback plays a significant role in influencing the properties of gas within their host galaxy and the circumgalactic medium.
Zhi-Fu Chen, Luis C. Ho
doaj +1 more source
A repeating fast radio burst associated with a persistent radio source. [PDF]
Niu CH +34 more
europepmc +1 more source
Dust Survival in Galactic Winds
We present a suite of high-resolution numerical simulations to study the evolution and survival of dust in hot galactic winds. We implement a novel dust framework in the Cholla hydrodynamics code and use wind tunnel simulations of cool, dusty clouds to ...
Helena M. Richie +3 more
doaj +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
We report the small-scale spatial variation in cool ( T ∼ 10 ^4 K) Mg ii absorption detected in the circumgalactic medium (CGM) of a star-forming galaxy at z ≈ 0.8.
Ahmed Shaban +8 more
doaj +1 more source
Quasars Probing Quasars: The Circumgalactic Medium Surrounding z ~ 2 Quasars [PDF]
Models of galaxy formation make the most direct predictions on gas related processes. Specifically, a picture on how gas flows through dark matter halos and onto galaxies to fuel star formation.
Lau, Marie Wingyee
core
Deep Ultraviolet, Emission-line Imaging of the Makani Galactic Wind
The O vi 1032, 1038 Å line is a key probe of cooling gas in the circumgalactic medium (CGM) of galaxies but has been observed to date primarily in absorption along single sight lines.
Triet Ha +16 more
doaj +1 more source
We present the Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic medium (DIISC) Survey. This survey is designed to investigate the correlations in properties between the circumgalactic medium (CGM), the interstellar
Fox, Andrew J. +15 more
core

