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Origin of galactic and extragalactic magnetic fields
LM Widrow - Reviews of Modern Physics, 2002 - APS
A variety of observations suggest that magnetic fields are present in all galaxies and galaxy
clusters. These fields are characterized by a modest strength (10− 7–10− 5 G) and huge …
clusters. These fields are characterized by a modest strength (10− 7–10− 5 G) and huge …
The origin and evolution of cosmic magnetism
BM Gaensler, R Beck, L Feretti - New Astronomy Reviews, 2004 - Elsevier
Magnetism is one of the four fundamental forces. However, the origin of magnetic fields in
stars, galaxies and clusters is an open problem in astrophysics and fundamental physics …
stars, galaxies and clusters is an open problem in astrophysics and fundamental physics …
A new model of the galactic magnetic field
R Jansson, GR Farrar - The Astrophysical Journal, 2012 - iopscience.iop.org
ABSTRACT A new, much-improved model of the Galactic magnetic field (GMF) is presented.
We use the WMAP7 Galactic synchrotron emission map and more than 40,000 extragalactic …
We use the WMAP7 Galactic synchrotron emission map and more than 40,000 extragalactic …
The galactic Faraday rotation sky 2020
Aims. This work provides an update to existing reconstructions of the Galactic Faraday
rotation sky by processing almost all Faraday rotation data sets available at the end of the …
rotation sky by processing almost all Faraday rotation data sets available at the end of the …
Science with the murchison widefield array
Significant new opportunities for astrophysics and cosmology have been identified at low
radio frequencies. The Murchison Widefield Array is the first telescope in the southern …
radio frequencies. The Murchison Widefield Array is the first telescope in the southern …
Detection of polarization in the cosmic microwave background using DASI
JM Kovac, EM Leitch, C Pryke, JE Carlstrom… - Nature, 2002 - nature.com
The past several years have seen the emergence of a standard cosmological model, in
which small temperature differences in the cosmic microwave background (CMB) radiation …
which small temperature differences in the cosmic microwave background (CMB) radiation …
The Canadian galactic plane survey
AR Taylor, SJ Gibson, M Peracaula… - The Astronomical …, 2003 - iopscience.iop.org
ABSTRACT The Canadian Galactic Plane Survey (CGPS) is a project to combine radio,
millimeter, and infrared surveys of the Galactic plane to provide arcminute-scale images of …
millimeter, and infrared surveys of the Galactic plane to provide arcminute-scale images of …
A rotation measure image of the sky
AR Taylor, JM Stil, C Sunstrum - The Astrophysical Journal, 2009 - iopscience.iop.org
We have re-analyzed the NRAO VLA Sky Survey (NVSS) data to derive rotation measures
(RMs) toward 37,543 polarized radio sources. The resulting catalog of RM values covers the …
(RMs) toward 37,543 polarized radio sources. The resulting catalog of RM values covers the …
Radio observational constraints on Galactic 3D-emission models
Context. Our position inside the Galaxy requires 3D-modelling to obtain the distribution of
the Galactic magnetic field, cosmic-ray (CR) electrons and thermal electrons. Aims. Our …
the Galactic magnetic field, cosmic-ray (CR) electrons and thermal electrons. Aims. Our …
Pulsar rotation measures and the large-scale structure of the galactic magnetic field
JL Han, RN Manchester, AG Lyne… - The Astrophysical …, 2006 - iopscience.iop.org
The large-scale magnetic field of our Galaxy can be probed in three dimensions using
Faraday rotation of pulsar signals. We report on the determination of 223 rotation measures …
Faraday rotation of pulsar signals. We report on the determination of 223 rotation measures …