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
Modelling Galaxies with a Multi-Phase ISM in 3d
We present a modified TREESPH code to model galaxies in 3d. The model includes a multi-phase description of the interstellar medium which combines two numerical techniques. A diffuse warm/hot gas phase is modelled by SPH while a sticky particle scheme is used to represent a cloudy medium.
Harfst, S., Theis, C., Hensler, G.
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Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
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Models of the ISM in galaxy centers
Part I: M51 is observed at a wavelength of 850 mum, where most radiation is emitted by dust. We find prominent spiral arms and an underlying exponential disk. The properties of the disk and the arms are studied. Part II and III: Gas in Galaxy Centers is exposed to intense radiation from a starburst region, an Active Galactic Nucleus (AGN), or both. The
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Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S +7 more
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Simulations of multi-phase gas in and around galaxies. [PDF]
Gronke M, E Schneider E.
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The cosmic ray ionization and γ-ray budgets of star-forming galaxies. [PDF]
Krumholz MR, Crocker RM, Offner SSR.
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Discs no more: the morphology of low-mass simulated galaxies in FIREbox. [PDF]
Benavides JA +11 more
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Detection of companion galaxies around hot dust-obscured hyper-luminous galaxy W0410-0913. [PDF]
Ginolfi M +20 more
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Galaxy Evolution with Manifold Learning. [PDF]
Takeuchi TT, Cooray S, Kano RR.
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