[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 32] Re: triple outburst of GO Com
- Date: Thu, 6 Feb 1997 18:17:10 +0000 (GMT)
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Erik Kuulkers <e.kuulkers1@physics.oxford.ac.uk>
- Subject: [vsnet-chat 32] Re: triple outburst of GO Com
- cc: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- In-Reply-To: <199702061717.CAA02398@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Taichi Kato wrote:
> I believe V1028 Cyg has an outburst amplitude exceeding 6 magnitude
> based on the recent quiescent estimate. Doesn't it well deserve a TOAD?
> Or should we modify slightly the TOAD definition?
Defining a SU UMa star as a TOAD (or, equivalently, a WZ Sge star) SOLELY
basing it on outburst magnitude is not the right way to classify it as a
TOAD. In addition the star should exhibit long intervals between
superoutbursts (years to decades) with almost no normal outbursts.
Note that this does not imply that the TOADs should be regarded as a
completely new CV-group. They are most probably the extreme end of
normal SU UMa stars.
The bright superoutburst and subsequent rebrightenings in V1028 Cyg
occurred after a long quiescent period and may in this respect resemble
TOADs. However, this star also show periods of regular normal and
superoutburst behaviour.
V1028 Cyg, and a similar system, SW UMa, may be the bridge between
normal SU UMa's and TOADs.
Erik Kuulkers
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp