Further joint X-ray, infrared, and radio observations of Cygnus X-3

Details Further joint X-ray, infrared, and radio observations of Cygnus X-3 Further joint X-ray, infrared, and radio observations of Cygnus X-3

Jul 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...207...78m&link_type=abstract

Astrophysical Journal, vol. 207, July 1, 1976, pt. 1, p. 78-87.

Astronomy and Astrophysics

Astronomy

53

Infrared Radiation, Power Spectra, Radiant Flux Density, Radio Sources (Astronomy), X Ray Sources, Astronomical Models, Data Recording, Emission Spectra, Periodic Variations, Stellar Winds

Scientific paper

Observations of Cygnus X-3 have been carried out at 2.5-7.5 keV, 2.2 micrometers, 8.1 GHz, and 2.7 GHz over a two week period. The X-ray data show the periodic structure which is typical of Cyg X-3. At times the X-ray and infrared measurements show very similar periodic structure, both in phase and in shape, while at other times the infrared data show no periodic variability. The radio fluxes were unusually low during the period of observation; both the daily average radio flux levels and the spectral index remained nearly constant.

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