Eclipses in the Binary System V1343-AQUILAE = SS:433

Details Eclipses in the Binary System V1343-AQUILAE = SS:433 Eclipses in the Binary System V1343-AQUILAE = SS:433

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986atsir1422....1g&link_type=abstract

Astronomicheskii Tsirkulyar NO. 1422/FEB, 1986

Astronomy and Astrophysics

Astronomy

Scientific paper

The light standstill of 0P.07 - 0P.11 duration is found in the deepest minima of the eclipsing binary V1343 Aql (SS433), during which the star shows only weak light variations. It is nearly one third of the eclipse phase range. The loss of light in the eclipse is 50 per cent at the precession period phases ψ ≡ 0 when the object is brightest out of eclipse. The eclipse standstill level in the bright state in SS433 (at ψ ≡ 0p.8 - 0p.2) is the same as minimal out of the eclipse light level in the faint state (ψ ≡ 0p.4 - 0p.6) seen at orbital phases φ = 0P.6 - 0P.9. The results of V band optical monitoring of 1985 August 17 eclipse are given in a table.

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