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[vsnet-campaign-dn 3627] RX Vol: refined superhump period
- Date: Wed, 7 May 2003 11:57:12 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp,vsnet-superoutburst@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-campaign-dn 3627] RX Vol: refined superhump period
- Delivered-To: vsnet-campaign-dn-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
RX Vol: refined superhump period
Dear Colleagues,
We have received further data from Peter Nelson. There was no further
development of the superhump amplitude. The present peak amplitude
of the superhumps are slightly smaller than those of long-period SU UMa-type
dwarf novae, but is a more usual value for short-period (especially
WZ Sge-like) systems.
The refined superhump period of 0.06117(5) d. There has been
a marginal trend of a slight period decrease, but this needs to be
examined in detail by further observations.
Regards,
Taichi Kato
VSNET Collaboration team

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