IR variability of SS433

Details IR variability of SS433 IR variability of SS433

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.291..392c&link_type=abstract

Nature, Volume 291, Issue 5814, pp. 392-394 (1981).

Physics

12

Scientific paper

SS433 shows X-ray, optical and radio variability and evidence of material moving at one-quarter the speed of light1. We report here the presence of the 165.5-day spectroscopic period in our extensive JHKL (1.2-3.4 µm) photometry. This indicates that the jets, rather than a highly reddened O star, are a major source of the IR radiation. We also show that the (J-H) colour index becomes redder as SS433 brightens but find no evidence for the 11.8-day period reported by Giles et al.2.

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