Cosmic ray processes in galactic ecosystems
Galaxy evolution is an important topic, and our physical understanding must be complete to
establish a correct picture. This includes a thorough treatment of feedback. The effects of …
establish a correct picture. This includes a thorough treatment of feedback. The effects of …
Polarized thermal emission from dust in a galaxy at redshift 2.6
Magnetic fields are fundamental to the evolution of galaxies, playing a key role in the
astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic …
astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic …
The Pandora project–I. The impact of radiation, magnetic fields, and cosmic rays on the baryonic and dark matter properties of dwarf galaxies
S Martin-Alvarez, D Sijacki, MG Haehnelt… - Monthly Notices of …, 2023 - academic.oup.com
Enshrouded in several well-known controversies, dwarf galaxies have been extensively
studied to learn about the underlying cosmology, notwithstanding that physical processes …
studied to learn about the underlying cosmology, notwithstanding that physical processes …
Extragalactic magnetism with SOFIA (SALSA Legacy Program): the magnetic fields in the multiphase interstellar medium of the antennae galaxies
E Lopez-Rodriguez, AS Borlaff, R Beck… - The Astrophysical …, 2022 - iopscience.iop.org
Mergers are thought to be a fundamental channel for galaxy growth, perturbing the gas
dynamics and the magnetic fields (B-fields) in the interstellar medium (ISM). However, the …
dynamics and the magnetic fields (B-fields) in the interstellar medium (ISM). However, the …
Extragalactic Magnetism with SOFIA (SALSA Legacy Program). V. First Results on the Magnetic Field Orientation of Galaxies
AS Borlaff, E Lopez-Rodriguez, R Beck… - The Astrophysical …, 2023 - iopscience.iop.org
We present the analysis of the magnetic field (B-field) structure of galaxies measured with far-
infrared (FIR) and radio (3 and 6 cm) polarimetric observations. We use the first data release …
infrared (FIR) and radio (3 and 6 cm) polarimetric observations. We use the first data release …
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Gas and dust in nearby galaxies
Understanding the physical processes that regulate star formation and galaxy evolution are
major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to …
major areas of activity in modern astrophysics. Nearby galaxies offer unique opportunities to …
The magnetic fields of starburst galaxies. I. Identification and characterization of the thermal polarization in the galactic disk and outflow
E Lopez-Rodriguez - The Astrophysical Journal, 2023 - iopscience.iop.org
Far-infrared polarized emission by means of magnetically aligned dust grains is an excellent
tracer of the magnetic fields (B-fields) in the cold phase of the galactic outflows of starburst …
tracer of the magnetic fields (B-fields) in the cold phase of the galactic outflows of starburst …
H i filaments as potential compass needles? Comparing the magnetic field structure of the Small Magellanic Cloud to the orientation of GASKAP-H i filaments
YK Ma, NM McClure-Griffiths, SE Clark… - Monthly Notices of …, 2023 - academic.oup.com
High-spatial-resolution H i observations have led to the realization that the nearby (within
few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the ambient …
few hundreds of parsecs) Galactic atomic filamentary structures are aligned with the ambient …
The structure of magnetic fields in spiral galaxies: a radio and far-infrared polarimetric analysis
WJ Surgent, E Lopez-Rodriguez… - The Astrophysical …, 2023 - iopscience.iop.org
We propose and apply a method to quantify the morphology of the large-scale ordered
magnetic fields (B-fields) in galaxies. This method is adapted from the analysis of Event …
magnetic fields (B-fields) in galaxies. This method is adapted from the analysis of Event …
Mapping and characterizing magnetic fields in the Rho Ophiuchus-A molecular cloud with SOFIA/HAWC+
Context. Together with gravity, turbulence, and stellar feedback, magnetic fields (B-fields)
are thought to play a critical role in the evolution of molecular clouds and star formation …
are thought to play a critical role in the evolution of molecular clouds and star formation …