WSRT observations of radio sources in the galactic plane near l =54°

1986 ◽  
Vol 7 (2) ◽  
pp. 105-112 ◽  
Author(s):  
T. Velusamy ◽  
W. M. Goss ◽  
E. M. Arnal
Keyword(s):  
Galactic Plane ◽  
Radio Sources

scholarly journals The magnetic structure of our Galaxy: a review of observations

2008 ◽  
Vol 4 (S259) ◽  
pp. 455-466 ◽  
Author(s):  
JinLin Han
Keyword(s):  
Magnetic Fields ◽  
Magnetic Structure ◽  
Large Scale ◽  
Galactic Halo ◽  
Galactic Center ◽  
Galactic Plane ◽  
Galactic Disk ◽  
Dust Emission ◽  
Measure Data ◽  
Radio Sources

AbstractThe magnetic structure in the Galactic disk, the Galactic center and the Galactic halo can be delineated more clearly than ever before. In the Galactic disk, the magnetic structure has been revealed by starlight polarization within 2 or 3 kpc of the Solar vicinity, by the distribution of the Zeeman splitting of OH masers in two or three nearby spiral arms, and by pulsar dispersion measures and rotation measures in nearly half of the disk. The polarized thermal dust emission of clouds at infrared, mm and submm wavelengths and the diffuse synchrotron emission are also related to the large-scale magnetic field in the disk. The rotation measures of extragalactic radio sources at low Galactic latitudes can be modeled by electron distributions and large-scale magnetic fields. The statistical properties of the magnetized interstellar medium at various scales have been studied using rotation measure data and polarization data. In the Galactic center, the non-thermal filaments indicate poloidal fields. There is no consensus on the field strength, maybe mG, maybe tens of μG. The polarized dust emission and much enhanced rotation measures of background radio sources are probably related to toroidal fields. In the Galactic halo, the antisymmetric RM sky reveals large-scale toroidal fields with reversed directions above and below the Galactic plane. Magnetic fields from all parts of our Galaxy are connected to form a global field structure. More observations are needed to explore the untouched regions and delineate how fields in different parts are connected.

scholarly journals A Catalogue of Galactic Radio Sources

1968 ◽  
Vol 21 (3) ◽  
pp. 369 ◽  
Author(s):  
MJL Kesteven
Keyword(s):  
Flux Density ◽  
Spectral Index ◽  
Galactic Plane ◽  
Radio Sources ◽  
Galactic Radio

The results of a survey of radio sources in the galactic plane in the longitude range 1800 to 400 with the 1 mile Molonglo Cross telescope at 408 MHz are presented. The methods of observation and reduction are described briefly. The catalogue lists the position, flux density, size, and spectral index for 80 sources

VLA observations of compact radio sources near the galactic plane

1983 ◽  
Vol 204 (2) ◽  
pp. 647-654 ◽  
Author(s):  
J. J. Rickard ◽  
W. C. Erickson ◽  
R. A. Perley ◽  
W. M. Cronynt
Keyword(s):  
Galactic Plane ◽  
Radio Sources

VLA structure of variable radio sources in the Galactic plane

1988 ◽  
Vol 95 ◽  
pp. 1149 ◽  
Author(s):  
Nebojsa Duric ◽  
P. C. Gregory
Keyword(s):  
Galactic Plane ◽  
Radio Sources ◽  
Variable Radio

Compact radio sources in the galactic plane

1988 ◽  
Vol 328 ◽  
pp. 559 ◽  
Author(s):  
Terry Jay Jones ◽  
Robert Garwood ◽  
John M. Dickey
Keyword(s):  
Galactic Plane ◽  
Radio Sources

Compact radio sources near the Galactic plane

1992 ◽  
Vol 80 ◽  
pp. 211 ◽  
Author(s):  
D. J. Helfand ◽  
S. Zoonematkermani ◽  
R. H. Becker ◽  
R. L. White
Keyword(s):  
Galactic Plane ◽  
Radio Sources

A catalog of small-diameter radio sources in the Galactic plane

1990 ◽  
Vol 74 ◽  
pp. 181 ◽  
Author(s):  
S. Zoonematkermani ◽  
D. J. Helfand ◽  
R. H. Becker ◽  
R. L. White ◽  
R. A. Perley
Keyword(s):  
Galactic Plane ◽  
Small Diameter ◽  
Radio Sources

scholarly journals Extended Polarized Emission Structures in the Galactic Plane at 11 cm Wavelength

1990 ◽  
Vol 140 ◽  
pp. 63-64
Author(s):  
N. Junkes ◽  
E. Fürst ◽  
W. Reich
Keyword(s):  
Supernova Remnants ◽  
Spiral Structure ◽  
Galactic Plane ◽  
Radio Sources ◽  
Galactic Magnetic Field ◽  
Background Component ◽  
Polarized Emission ◽  
The Galaxy ◽  
Galactic Longitude ◽  
Thermal Background

Data from the Effelsberg Galactic plane survey at 11 cm wavelength have been used to produce a survey of polarized intensity in the first Galactic quadrant. Besides polarized sources (Supernova remnants and extragalactic objects) extended polarized emission features are visible, which are not connected to distinct radio sources. To decide whether these features reflect characteristics of the local field or the distant spiral structure of the Galaxy we performed an integration of polarized intensities as a function of Galactic longitude. An anticorrelation with the thermal background component suggests a distance of more than 6 kpc for some components of the polarized emission. This enables us to derive an upper limit for the uniform component of the Galactic magnetic field.

scholarly journals VARIABLE RADIO SOURCES IN THE GALACTIC PLANE

2010 ◽  
Vol 140 (1) ◽  
pp. 157-166 ◽  
Author(s):  
Robert H. Becker ◽  
David J. Helfand ◽  
Richard L. White ◽  
Deanne D. Proctor
Keyword(s):  
Galactic Plane ◽  
Radio Sources ◽  
Variable Radio
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