Low frequency polarization observations of the Galactic radio emission

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 alpha 1950 = 4h 30m, beta 1950 = 61 deg reveals a nonmonotonic, oscillating spectrum of the po...

Full description

Saved in:
Bibliographic Details
Main Authors: Vinyajkin, E N, Razin, V A
Format: Conference Proceeding
Language:English
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
Description
Summary: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 alpha 1950 = 4h 30m, beta 1950 = 61 deg reveals a nonmonotonic, oscillating spectrum of the polarized brightness temperature. On the contrary, the region of the North Celestial Pole (l=123 deg, b= 27 deg 24 arcmin) has practically monotonic spectrum. The possible reasons for this difference are discussed. (Author)
ISSN:0094-243X