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[vsnet-chat 85] Re: EG Cnc - first one?
- Date: Mon, 17 Feb 1997 11:55:50 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 85] Re: EG Cnc - first one?
- Cc: astroman@voyager.co.nz, fraserf@dove.net.au
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Fraser Farrell wrote:
> I speculate that EG Cnc may represent an extreme example - decades of
> inactivity, then months (years??) of vigorous activity, then inactivity
> again. Perhaps this should be part of the definition of ER UMa stars?
> I await discussion from our professional readers!
I believe the ER UMa stars are defined by their short supercycle
lengths, and not by activity/inactivity cycles. ER UMa stars are assumed
to have exceptionally high mass-transfer rates among SU UMa-type dwarf
novae, in contrast to EG Cnc or WZ Sge-stars. However, it is still
under investigation whether secular changes exist in ER UMa stars.
I hope Nogami-san has some comments on this matter.
Regards,
Taichi Kato
Return to Daisaku Nogami
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