The Galactic latitude dependence of centimeter-wavelength flicker

Details The Galactic latitude dependence of centimeter-wavelength flicker The Galactic latitude dependence of centimeter-wavelength flicker

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987aj.....93..589h&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 93, March 1987, p. 589-591.

Astronomy and Astrophysics

Astronomy

23

Centimeter Waves, Extragalactic Radio Sources, Scintillation, Amplitudes, Latitude, Radiant Flux Density

Scientific paper

Small-amplitude flickering of the flux density of extragalactic radio sources has been found at 9 cm by Heeschen (1984). It that paper, it was concluded that there was no apparent dependence of the flicker on Galactic latitude. Here, all the pertinent 9 cm data are reanalyzed, and it is found that flicker amplitude does show a latitude dependence consistent with that expected from interstellar scintillation.

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