An anomaly in the flux of Cassiopeia A at 38 MHz

Details An anomaly in the flux of Cassiopeia A at 38 MHz An anomaly in the flux of Cassiopeia A at 38 MHz

Sep 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...200l..83e&link_type=abstract

Astrophysical Journal, vol. 200, Sept. 1, 1975, pt. 2, p. L83-L87.

Astronomy and Astrophysics

Astronomy

28

Cassiopeia A, Radiant Flux Density, Secular Variations, Supernova Remnants, Abnormalities, Radio Astronomy, Radio Emission, Radio Sources (Astronomy), Radio Spectra

Scientific paper

The secular decrease in the flux of the supernova remnant Cassiopeia A
has been measured at many radio frequencies. Observations are reported
which indicate that this flux decrease has halted at 38 MHz and that the
flux is increasing at this frequency. This may indicate that a new era
of activity has begun in this object.

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