The origin of the diverse morphologies and kinematics of Milky Way-mass galaxies in the FIRE-2 simulations. [PDF]
Garrison-Kimmel S +13 more
europepmc +1 more source
Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions. [PDF]
Famaey B, McGaugh SS.
europepmc +1 more source
Mapping Galactic Winds and Small-scale Structure in the Circumgalactic Medium with Habitable Worlds Observatory [PDF]
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]
Ahmed Shaban +8 more
openalex +1 more source
Unveiling the Complex Circumgalactic Medium: A Comparative Study of Merging and Non-Interacting Galaxy Groups [PDF]
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
Pérez-González P +21 more
europepmc +1 more source
Related searches:
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 JournalWe 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 SocietyCosmic 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

