Low frequency polarization observations of the galactic radio emission

Details Low frequency polarization observations of the galactic radio emission Low frequency polarization observations of the galactic radio emission

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..609...26v&link_type=abstract

ASTROPHYSICAL POLARIZED BACKGROUNDS: Workshop on Astrophysical Polarized Backgrounds, held 9-12 October, 2001 in Bologna Italy.

Physics

4

Radiation Mechanisms, Polarization, Physical Properties, Radio, Microwave, Characteristics And Properties Of The Milky Way Galaxy

Scientific paper

Multifrequency polarization observations of a number of regions of the Galaxy in the frequency range 200-1250 MHz have been carried out. The area of enhanced linear polarization at meter wavelengths around α1950=4h30m, δ1950=61° (l=146°47',b=9°03') reveals a nonmonotonic, oscillating spectrum of the polarized brightness temperature. On the contrary, the region of the North Celestial Pole (l=123°,b=27°24') has practically monotonic spectrum. The possible reasons for this difference are discussed. .

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