Results 71 to 80 of about 437 (157)
Fast radio bursts (FRBs) are luminous, millisecond-duration transients that offer great potential for probing the Universe, yet their physical origins remain unclear.
Jian-feng Mo +2 more
doaj +1 more source
DIISC-VI (COS-DIISC): Ultraviolet Metal Absorption Relative to the H i Disk of Galaxies
As part of the Deciphering the Interplay between the Interstellar medium, Stars, and the Circumgalactic medium (DIISC) survey, we present the UV metal absorption features in the circumgalactic medium (CGM) near the H i gas disk (
Brad Koplitz +7 more
doaj +1 more source
Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913. [PDF]
Ginolfi M +20 more
europepmc +1 more source
THE HIGHLY IONIZED CIRCUMGALACTIC MEDIUM IS KINEMATICALLY UNIFORM AROUND GALAXIES
ABSTRACT The circumgalactic medium (CGM) traced by O vi doublet absorption has been found to concentrate along the projected major and minor axes of the host galaxies. This suggests that O vi traces accreting and outflowing gas, respectively, which are key components of ...
Nikole M. Nielsen +5 more
openaire +5 more sources
The Signatures of Density Fluctuations and Mixing Gas in Circumgalactic Absorption Systems
We investigate the prospects for detecting and constraining density and temperature inhomogeneities in the circumgalactic medium using absorption measurements of metal ions.
Yakov Faerman +3 more
doaj +1 more source
Phosphorus-bearing molecules PO and PN at the edge of the Galaxy. [PDF]
Koelemay LA, Gold KR, Ziurys LM.
europepmc +1 more source
In dwarf galaxy models, outflows expel metal-enriched interstellar medium (ISM) into the circumgalactic medium (CGM) to reproduce their observed low metallicities, but measurements of dwarf CGM properties are scarce.
Sean D. Johnson +15 more
doaj +1 more source
The origin of cold gas in the circumgalactic medium
Context. The presence of cold gas (T ≲ 104 K) in the circumgalactic medium (CGM) of galaxies has been confirmed in observations and in high-resolution simulations, but its origin is still a puzzle. Possible mechanisms are cold accretion from the intergalactic medium (IGM), clumps embedded in outflows and transported from the disk, and gas detaching ...
Decataldo, Davide +4 more
openaire +4 more sources
Mapping the z ∼ 2 Circumgalactic Medium with KBSS Galaxy Pairs
We present new results on the spatial structure and kinematics of the circumgalactic medium (CGM) of z ∼ 2 star-forming galaxies drawn from the Keck Baryonic Structure Survey, using Ly α and metallic ion absorption recorded in spectra of background ...
Nikolaus Z. Prusinski +2 more
doaj +1 more source
Understanding the circumgalactic medium (CGM) distribution of galaxies is the key to revealing the dynamical exchange of materials between galaxies and their surroundings.
Zeyu Chen +12 more
doaj +1 more source

