Volume 621, January 2019
|Number of page(s)||13|
|Section||Interstellar and circumstellar matter|
|Published online||17 January 2019|
Low-frequency measurements of synchrotron absorbing HII regions and modeling of observed synchrotron emissivity
Department of Astrophysics/IMAPP, Radboud University,
PO Box 9010,
2 CRESST II, NASA Goddard Space Flight Center, Greenbelt, MD, 20771, USA
3 Department of Astronomy, University of Maryland, College Park, MD, 20742, USA
Accepted: 24 November 2018
Context. Cosmic rays (CRs) and magnetic fields are dynamically important components in the Galaxy, and their energy densities are comparable to that of the turbulent interstellar gas. The interaction of CRs and Galactic magnetic fields (GMF) produces synchrotron radiation clearly visible in the radio regime. Detailed measurements of synchrotron radiation averaged over the line-of-sight (LOS), so-called synchrotron emissivities, can be used as a tracer of the CR density and GMF strength.
Aims. Our aim is to model the synchrotron emissivity in the Milky Way using a three-dimensional dataset instead of LOS-integrated intensity maps on the sky.
Methods. Using absorbed HII regions, we measured the synchrotron emissivity over a part of the LOS through the Galaxy, changing from a two-dimensional to a three-dimensional view. Performing these measurements on a large scale is one of the new applications of the window opened by current low-frequency arrays. Using various simple axisymmetric emissivity models and a number of GMF-based emissivity models, we were able to simulate the synchrotron emissivities and compare them to the observed values in the catalog.
Results. We present a catalog of low-frequency absorption measurements of HII regions, their distances and electron temperatures, compiled from literature. These data show that the axisymmetric emissivity models are not complex enough, but the GMF-based emissivity models deliver a reasonable fit. These models suggest that the fit can be improved by either an enhanced synchrotron emissivity in the outer reaches of the Milky Way or an emissivity drop near the Galactic center.
Conclusions. Current GMF models plus a constant CR density model cannot explain low-frequency absorption measurements, but the fits improved with slight (ad hoc) adaptations. It is clear that more detailed models are needed, but the current results are very promising.
Key words: cosmic rays / ISM: magnetic fields / HII regions / Galaxy: structure / radio continuum: ISM / catalogs
© ESO 2019
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