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[vsnet-alert 6443] Re: WZ Sge: new hump structure and possible QPOs
- Date: Sun, 26 Aug 2001 05:27:33 +0200
- To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- From: Gianluca Masi <gianmasi@fr.flashnet.it>
- Subject: [vsnet-alert 6443] Re: WZ Sge: new hump structure and possible QPOs
- CC: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign@kusastro.kyoto-u.ac.jp, vsnet-superoutburst@kusastro.kyoto-u.ac.jp
- Organization: "Bellatrix" Astronomical Observatory
- References: <200108260327.MAA06329@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Taichi Kato wrote:
>
> WZ Sge: new hump structure and possible QPOs
>
> Dear Colleagues,
>
> The analysis of the latest data (J. Pietz and A. Oksanen) has revealed
> the emergence of new (super)humps at phases completely different from
> the previous superhumps (during the second rebrightening). This phenomenon
> may be some sort of "late superhumps" to newly appeared superhumps during
> the second rebrightening (how complex!). There seem to be no "true" eclipse
> signals.
>
> Furthermore, large-amplitude modulations with time-scales of ~20 min.
> Although they may be substuctures of (super)hump signals, they may represent
> the emergence of new QPOs. Since some super-QPOs are known to arise from
> these slow modulations (cf. EF Peg in 1991), observers are strongly urged
> to record the evolution of short-term oscillations, as well as evolution
> of (super)humps.
>
Dear Taichi,
this actually confirms what I reported in vsnet-campaign-dn 1369 (also sent to
vsnet alert, but still not distribuited)! A very nice finding!
Regards,
Gianluca
--
***********************************************************************
* Gianluca Masi "Two things fill the soul *
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* e-mail: gianmasi@fr.flashnet.it *
* web: http://vsnet.eurolink.it/comets/ I. Kant *
* Minor Planet Center Obs. Code: 470 - Ceccano *
* Center for Backyard Astrophysics - Italy *
* VSNET Collaboration Team member *
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