Results 181 to 190 of about 3,496,469 (217)
Higher-order sonification of the human brain. [PDF]
Sci RepKitaura FS +5 more
europepmc +1 more source
Unravelling the Origin of Magnetic Fields in Galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2021 ABSTRACT Despite their ubiquity, there are many open questions regarding galactic and cosmic magnetic fields. Specifically, current observational constraints cannot rule out whether magnetic fields observed in galaxies were generated in the early Universe or are of astrophysical nature.
Debora Šijački +2 more
exaly +5 more sources
Magnetic Fields in Clusters of Galaxies [PDF]
International Journal of Modern Physics D, 2004 The existence of magnetic fields associated with the intracluster medium in clusters of galaxies is now well established through different methods of analysis. Magnetic fields are investigated in the radio band from studies of the rotation measure of polarized radio galaxies and the synchrotron emission of cluster-wide diffuse sources.
Federica Govoni, Luigina Feretti
exaly +6 more sources
Magnetic Field Amplification in Young Galaxies [PDF]
Astronomy and Astrophysics, 2013 13 pages, 8 figures; A&A in ...
Ralf Klessen
exaly +4 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
Astronomy and Astrophysics Review, 1993
Recent years have seen an amazing development in our knowledge of the magnetic fields in the universe. The last ten years were crucial in our realization of the importance of the magnetic fields in galaxies. While a lot of the earlier data on our Galaxy depended on optical observations, the bulk of the recent results depend on radio measurements.
R Wielebinski, F Krause
exaly +2 more sources
Recent years have seen an amazing development in our knowledge of the magnetic fields in the universe. The last ten years were crucial in our realization of the importance of the magnetic fields in galaxies. While a lot of the earlier data on our Galaxy depended on optical observations, the bulk of the recent results depend on radio measurements.
R Wielebinski, F Krause
exaly +2 more sources
Geophysical & Astrophysical Fluid Dynamics, 1987
The observations of the optical polarization of starlight [1,2] showed large-scale alignment of the vectors which was interpreted to be due to galactic magnetic fields which align interstellar grains [3]. The data on star polarization accumulated over many years (e.g. [4,5,6]) giving in the end a large sample of objects at known distances.
openaire +1 more source
The observations of the optical polarization of starlight [1,2] showed large-scale alignment of the vectors which was interpreted to be due to galactic magnetic fields which align interstellar grains [3]. The data on star polarization accumulated over many years (e.g. [4,5,6]) giving in the end a large sample of objects at known distances.
openaire +1 more source
Magnetic fields in the galaxy and galaxies
EAS Publications Series, 2005Magnetic fields are found everywhere in the cosmic Universe. They have been known to exist on the Earth for centuries. They were detected in the Sun, measured in situ in the planets, observed in stars, galaxies and clusters of galaxies. Magnetic fields are responsible for many observed effects like radio continuum emission, jets, beamed emission in ...
openaire +1 more source
2014
The hadronic constituent of galaxies consists of gas and stars, with only a minor contribution of dust. These components rotate in a gravitational potential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase.
Ulrich Klein, Andrew Fletcher
openaire +1 more source
The hadronic constituent of galaxies consists of gas and stars, with only a minor contribution of dust. These components rotate in a gravitational potential made up by stars and dark matter. In spiral galaxies, the gas has a neutral and an ionised phase.
Ulrich Klein, Andrew Fletcher
openaire +1 more source