Observed properties of the interstellar magnetic field

Details Observed properties of the interstellar magnetic field Observed properties of the interstellar magnetic field

May 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974mmsai..45...61a&link_type=abstract

(Ministero della Pubblica Istruzione, CNR, and Universita di Trieste, European Regional Meeting in Astronomy, 2nd, Trieste, Ital

Astronomy and Astrophysics

Astronomy

2

Hydrogen Clouds, Interstellar Gas, Interstellar Magnetic Fields, Magnetic Flux, Flow Distribution, Galactic Evolution, Galactic Rotation, Gas Density, Gas Dynamics, Gas Flow, Spiral Galaxies, Star Clusters, Synchrotron Radiation

Scientific paper

The paper reviews present knowledge of the field strength, large scale structure and small scale structure of the interstellar magnetic field. Field strength in interstellar H I clouds is plotted as a function of the hydrogen density. Large scale structure is studied for the Cygnus region and the north galactic pole on the basis of interstellar polarization. Small scale structure is studied near the alpha Persei cluster and in the Orion aggregate also on the basis of interstellar polarization.

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