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[vsnet-chat 3879] Re: [vsnet-outburst 1196] RZ Leo - a new UGSU type variable !!!
- Date: Thu, 21 Dec 2000 20:35:33 +0100
- To: Tonny Vanmunster <Tonny.Vanmunster@advalvas.be>, VSNET <vsnet-chat@kusastro.kyoto-u.ac.jp>
- From: Thorsten Lange <tl@thola.de>
- Subject: [vsnet-chat 3879] Re: [vsnet-outburst 1196] RZ Leo - a new UGSU type variable !!!
- In-Reply-To: <NBBBJKIECBCGIADLBIHHMEMPDMAA.Tonny.Vanmunster@advalvas.be>; from Tonny.Vanmunster@advalvas.be on Thu, Dec 21, 2000 at 09:25:53AM +0100
- References: <NBBBJKIECBCGIADLBIHHMEMPDMAA.Tonny.Vanmunster@advalvas.be>
- Reply-To: tl@thola.de
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Hello,
> The above observations thus establish RZ Leo as yet another new member of
> the UGSU type of cataclysmic variables !
It seems to me, that everytime (?) when somebody observers such stars with
high-speed photometry, a superhump period is detected. Is is possible, that
all those stars are UGSU? Or do I mix facts that don't fit together?
Is there something in the live of cataclysmic stars which depends on the
amplitude and/or period and/or superhump itself?
Thorsten Lange
--
Thorsten Lange
EMail tl@thola.de
http://thola.de/
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