Results 21 to 30 of about 1,565,970 (180)
The Anisotropic Circumgalactic Medium of Sub-L* Galaxies
Using stacked emission-line flux measurements of cool circumgalactic gas (CGM) in lower-mass galaxies (10 ^9.0 ≤ M _* / M _⊙ ≤ 10 ^10.2 ), we measure the dependence of the emission characteristics on orientation relative to the disk plane as a function ...
Huanian Zhang, Miao Li, Dennis Zaritsky
doaj +3 more sources
Key Physical Processes in the Circumgalactic Medium [PDF]
Spurred by rich, multiwavelength observations and enabled by new simulations, ranging from cosmological to subparsec scales, the past decade has seen major theoretical progress in our understanding of the circumgalactic medium (CGM). We review key physical processes in the CGM. Our conclusions include the following: ▪The properties of the CGM depend on
Faucher-Giguere, Claude-Andre +1 more
openaire +3 more sources
The MUSECuBES surveys on the circumgalactic medium
The circumgalactic medium (CGM) is a dynamic, complex, multiphase, metal-enriched gas reservoir surrounding galaxies which harbors gas and metal masses comparable to those in galaxies themselves. Using a large quantity of spectral and imaging data obtained with MUSE & UVES on the VLT and ACS & COS on-board HST, we have started a major campaign ...
Muzahid, Sowgat (6471758) +1 more
openaire +3 more sources
Understanding gas mixing in the circumgalactic medium [PDF]
ABSTRACT We study gas mixing in a simulated Milky Way–mass galaxy’s circumgalactic medium (CGM) using cosmological ‘zoom-in’ simulations. We insert tracer dyes in the CGM with different gas flows (shearing, coherent, and static) and diverse physical properties to track gas mixing.
Hilay Shah +3 more
openaire +3 more sources
Making the Deepest Images of the Circumgalactic Medium
Abstract The aim of this research is to utilise data from the IMAGINE survey to probe deeper into the circumgalactic medium (CGM) of spiral galaxy NGC7424 and identify large scale HI structures using the high column densities achievable with ATCA.
Tasmiyah Rawoot, D.J. Pisano
openaire +2 more sources
The Truncated Circumgalactic Medium of the Large Magellanic Cloud
The Large Magellanic Cloud (LMC) is the nearest massive galaxy to the Milky Way (MW). Its circumgalactic medium (CGM) is complex and multiphase, containing both stripped H i structures like the Magellanic Stream and Bridge and a diffuse warm corona seen ...
Sapna Mishra +8 more
doaj +3 more sources
Properties of the simulated circumgalactic medium [PDF]
ABSTRACT The circumgalactic medium (CGM) is closely linked to galaxy formation and evolution, but difficult to characterize observationally and typically poorly resolved in cosmological simulations. We use spherically symmetric, idealized, high-resolution simulations of the CGM in $10^{12}$ and $10^{11}\, \mathrm{M}_\odot$ dark matter ...
Cassandra Lochhaas +4 more
openaire +2 more sources
THE INFLUENCE OF ENVIRONMENT ON THE CIRCUMGALACTIC MEDIUM [PDF]
The effect of environment on the circumgalactic medium (CGM) is investigated through a comparison of Lya absorption line data in the Virgo Cluster and the field. This Letter uses the first systematic survey of background QSOs in and around the Virgo Cluster and large existing surveys of galaxies at low redshift. While previous studies found denser gas (
Yoon, Joo Heon, Putman, Mary
openaire +2 more sources
Project AMIGA: The Circumgalactic Medium of Andromeda* [PDF]
Abstract Project AMIGA (Absorption Maps In the Gas of Andromeda) is a survey of the circumgalactic medium (CGM) of Andromeda (M31, ≃ 300 kpc) along 43 QSO sightlines at impact parameters 25 ≤ R ≤ 569 kpc (25 at R ≲
Nicolas Lehner +24 more
openaire +3 more sources
MUSE-ALMA Halos XI: Gas flows in the circumgalactic medium [PDF]
The flow of gas into and out of galaxies leaves traces in the circumgalactic medium which can then be studied using absorption lines towards background quasars. We analyse 27 log(N_HI) > 18.0 HI absorbers at z = 0.2 to 1.4 from the MUSE-ALMA Halos survey
Glenn G Kacprzak +45 more
core +1 more source

