Spectra and linear polarizations of extragalactic variable sources at centimeter wavelengths

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

320

Centimeter Waves, Extragalactic Radio Sources, Linear Polarization, Radiant Flux Density, Bl Lacertae Objects, Quasars, Radio Spectra

Scientific paper

The results of multifrequency observations of the flux densities and linear polarizations of 97 extragalactic sources obtained with the University of Michigan 26 m paraboloid through November 1984 are presented. The observations were started at 8.0 GHz in June 1965, at 14.5 GHz in February 1974, and at 4.8 GHz in September 1977. The data show that the degrees of polarization of these objects at centimeter wavelengths rarely exceed 15 percent and are typically on the order of 5 percent or less. In many, but not all, sources the observed variations are significantly faster and have a larger amplitude at the highest frequency. The majority of the sources appear to have preferred orientations of the electric vector of the polarized emission which exist over successive outbursts in total flux density.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Spectra and linear polarizations of extragalactic variable sources at centimeter wavelengths does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Spectra and linear polarizations of extragalactic variable sources at centimeter wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectra and linear polarizations of extragalactic variable sources at centimeter wavelengths will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1160567

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.