Non-variable 13.5 MM flux in the strong millimetre component of Centaurus A

Details Non-variable 13.5 MM flux in the strong millimetre component of Centaurus A Non-variable 13.5 MM flux in the strong millimetre component of Centaurus A

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975natur.254..124f&link_type=abstract

Nature, vol. 254, Mar. 13, 1975, p. 124, 125. Research supported by the Conselho Nacional de Pesquinas do Brazil, FADESP, and BN

Astronomy and Astrophysics

Astronomy

9

Microwave Emission, Millimeter Waves, Radiant Flux Density, Radio Galaxies, Infrared Astronomy, Periodic Variations, Radio Sources (Astronomy), Radio Telescopes, Statistical Analysis

Scientific paper

In the investigation reported, 18 measurements were made of Cen A at the position of the infrared source at a wavelength of 13.5 on nine days between April and December 1974. The observations were made with a 13.7-m radio telescope. The obtained data of the flux density are presented in a table together with observations of the reference source, Virgo A. No evidence for variability could be found at the considered wavelength during the times of observation.

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