Magnetic field and ISM in the local Galactic disc
Astrophysics of Galaxies
2019-08-29 v3
Abstract
Correlation analysis is obtained among Faraday rotation measure, HI column density, thermal and synchrotron radio brightness using archival all-sky maps of the Galaxy. A method is presented to calculate the magnetic strength and its line-of-sight (LOS) component, volume gas densities, effective LOS depth, effective scale height of the disk) from these data in a hybrid way. Applying the method to archival data, all-sky maps of the local magnetic field strength and its parallel component are obtained, which reveal details of local field orientation.
Keywords
Cite
@article{arxiv.1902.02535,
title = {Magnetic field and ISM in the local Galactic disc},
author = {Y. Sofue and H. Nakanishi and K. Ichiki},
journal= {arXiv preprint arXiv:1902.02535},
year = {2019}
}
Comments
11 pages, 15 figures, appeared in MNRAS, full resolution copy at http://www.ioa.s.u-tokyo.ac.jp/~sofue/papers/sofcomp/2019-mn-LocalMag.pdf