[vsnet-alert 15639] CSS J174033.5+414756: updated period of early superhumps, spectrum
Taichi Kato
tkato at kusastro.kyoto-u.ac.jp
Tue Apr 23 10:15:53 JST 2013
CSS J174033.5+414756: updated period of early superhumps, spectrum
Pavol A. Dubovsky and Colin Littlefield have reported
further observations (Dubovsky's first observations was
earlier than Littlefield's one). We now have a much refined
period of early superhumps: 0.04503(1) d.
The profile is asymmetric double humps and the full amplitude
is about 0.02 mag (mean).
According to ATEL 4999, ASAS-SN team detected this object
on April 19 at V=12.7. The object has been confirmed to be
hydrogen-rich, and it is not an AM CVn-type object.
I see that He II 4686 is in emission and helium is enhanced
as seen from the strength of He I lines.
The object is likely to have an evolved core in
the secondary (pre-AM CVn-type?), and measurement of superhump
excess is extremely important. Please follow this object
as continuously as possible to detect stage A and B superhumps
and see how they emerge.
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