[vsnet-outburst 19087] ASASSN-15ux: eclipsing WZ Sge-type
Taichi Kato
tkato at kusastro.kyoto-u.ac.jp
Mon Jan 18 11:13:09 JST 2016
ASASSN-15ux: eclipsing WZ Sge-type
As expected, this object started to show eclipses.
Report from Enrique de Miguel:
Excluding the JD 401 run, in which the superhump wave
nearly overrides the eclipse, the (orbital) ephemeris
I find is
HJD(min) = 400.3232(4) + 0.056107(7) E
using JD 400, 403, and 404 runs.
There is a strong interaction between the
superhump and orbital waves, and this results in a
strong beat. A more reliable value would require
covering several beat cycles.
Porb is consistent with the best estimate of the
periodicity of early superhumps, P_esh = 0.056092(4) d,
and the known observational fact that P_esh is essentially
equal to Porb.
Removing the eclipses, the resulting (mean) frequency
of the superhump wave since JD 400 is 17.547(6) c/d,
consistent with the value:
fsh = 17.544(7) c/d --> Psh = 0.056999(2) d
after timing the maxima of the superhump
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