Galactic interstellar filaments as probed by LOFAR and Planck
@article{Zaroubi2015GalacticIF, title={Galactic interstellar filaments as probed by LOFAR and Planck}, author={S. Zaroubi and V. Jeli{\'c} and A. Bruyn and F. Boulanger and A. Bracco and R. Kooistra and M. Alves and M. Brentjens and K. Ferri{\`e}re and T. Ghosh and L. Koopmans and F. Levrier and M. Miville-Desch{\^e}nes and L. Montier and V. Pandey and J. Soler}, journal={Monthly Notices of the Royal Astronomical Society}, year={2015}, volume={454} }
Recent Low-Frequency Array (LOFAR) observations at 115-175 MHz of a field at medium Galactic latitudes (centred at the bright quasar 3C196) have shown striking filamentary structures in polarization that extend over more than 4° across the sky. In addition, the Planck satellite has released full sky maps of the dust emission in polarization at 353 GHz. The LOFAR data resolve Faraday structures along the line of sight, whereas the Planck dust polarization maps probe the orientation of the sky… CONTINUE READING
20 Citations
Planck intermediate results XLIV. Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
- Physics
- 2016
- 44
- PDF
Mapping the Magnetic Interstellar Medium in Three Dimensions Over the Full Sky with Neutral Hydrogen.
- Physics
- 2019
- 13
- PDF
References
SHOWING 1-10 OF 17 REFERENCES
Studying Galactic interstellar turbulence through fluctuations in synchrotron emission. First LOFAR Galactic foreground detection
- Physics
- 2013
- 61
- PDF
Planck intermediate results. XIX. An overview of the polarized thermal emission from Galactic dust
- Physics
- 2014
- 213
- PDF
Initial LOFAR observations of epoch of reionization windows: II. Diffuse polarized emission in the ELAIS-N1 field
- Physics
- 2014
- 52
- PDF
Planck intermediate results. XX. Comparison of polarized thermal emission from Galactic dust with simulations of MHD turbulence
- Physics
- 2015
- 92
- PDF
Searching for Inflationary B-modes: Can dust emission properties be extrapolated from 350 GHz to 150 GHz?
- Physics
- 2014
- 25
- PDF