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[vsnet-obs 31362] RZ Leo superhump period from CBA observations
- Date: Thu, 28 Dec 2000 00:24:29 -0000
- To: "cba-news" <news@cba.phys.columbia.edu>
- From: "Tonny Vanmunster" <Tonny.Vanmunster@advalvas.be>
- Subject: [vsnet-obs 31362] RZ Leo superhump period from CBA observations
- Cc: "vsnet-obs" <vsnet-obs@kusastro.kyoto-u.ac.jp>, "Vsnet-Campaign" <vsnet-campaign@kusastro.kyoto-u.ac.jp>
- Importance: Normal
- Reply-To: <Tonny.Vanmunster@advalvas.be>
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Dear colleagues,
An analysis of recent RZ Leo observations obtained at a number of CBA
stations, combined with data supplied by Jochen Pietz, reveals a fairly
simple superhump signal at 0.0785 +- 0.0002 d (compared with Porb = 0.07604
+- 0.00012 d). This yields a fractional period excess of 3.3%, which is a
rather standard excess value.
Kind regards,
Tonny Vanmunster
on behalf of the CBA gang
Return to Daisaku Nogami
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