Near Infrared Observations of Cygnus X-3

Details Near Infrared Observations of Cygnus X-3 Near Infrared Observations of Cygnus X-3

Feb 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974natur.247..446b&link_type=abstract

Nature, Volume 247, Issue 5441, pp. 446-447 (1974).

Physics

3

Scientific paper

THE system known as Cygnus X-3 has been extensively studied at radio wavelengths (where it exhibits extraordinary variability1-3), in X rays (where it exhibits a 4.8 h period4-6), and in the infrared at 1.6 and 2.2 µm (where it also displays a 4.8 h period as well as large flares7,8). Attempts have also been made to detect Cyg X-3 in visual and near infrared wavelengths9,10. Here we present the results of a series of observations made at near infrared wavelengths, λeffective ~=0.85 µm on ten nights in July and August 1973.

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