Results 211 to 220 of about 2,374,498 (256)

The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations. [PDF]

open access: yesMon Not R Astron Soc, 2018
Garrison-Kimmel S   +13 more
europepmc   +1 more source

Mapping Galactic Winds and Small-scale Structure in the Circumgalactic Medium with Habitable Worlds Observatory [PDF]

open access: green
Joseph N. Burchett   +6 more
openalex  

Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$ [PDF]

open access: green
Ahmed Shaban   +8 more
openalex   +1 more source

Unveiling the Complex Circumgalactic Medium: A Comparative Study of Merging and Non-Interacting Galaxy Groups [PDF]

open access: green
Antonia Fernández-Figueroa   +7 more
openalex   +1 more source

Feedback mechanisms stopping the star formation in a pair of massive galaxies in the early Universe

open access: yes
Pérez-González P   +21 more
europepmc   +1 more source
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Cosmic Rays Masquerading as Hot CGM Gas: An Inverse-Compton Origin for Diffuse X-ray Emission in the Circumgalactic Medium

The Open Journal of Astrophysics
Observations from ROSAT and eROSITA have argued that Milky Way (MW), Andromeda, and lower-mass galaxies exhibit extended soft X-ray ( 1keV) diffuse halos out to radii R≳100kpc in the circumgalactic medium (CGM).
Philip F. Hopkins   +3 more
semanticscholar   +1 more source

Thermal Sunyaev–Zel’dovich Effect in the Circumgalactic Medium. II. Dependence on Star Formation

Astrophysical Journal
We measure the thermal Sunyaev–Zel’dovich effect in the circumgalactic medium (CGM) of ≈2.5 million M200 = 1012−14M⊙ WISE × DESI galaxies out to z = 1.2.
Sanskriti Das   +3 more
semanticscholar   +1 more source

Constraining cosmic ray transport models using circumgalactic medium properties and observables

Monthly notices of the Royal Astronomical Society
Cosmic rays (CRs) are a pivotal non-thermal component of galaxy formation and evolution. However, the intricacies of CR physics, particularly how they propagate in the circumgalactic medium (CGM), remain largely unconstrained.
Yue Samuel Lu   +5 more
semanticscholar   +1 more source

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