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[vsnet-chat 5285] Re: [vsnet-outburst 3787] VW Hyi brighter
- Date: Fri, 5 Apr 2002 15:26:28 +1200
- To: "Taichi Kato" <tkato@kusastro.kyoto-u.ac.jp>, <vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp>
- From: "Stan Walker" <astroman@xtra.co.nz>
- Subject: [vsnet-chat 5285] Re: [vsnet-outburst 3787] VW Hyi brighter
- Cc: <vsnet-chat@kusastro.kyoto-u.ac.jp>
- Delivered-To: vsnet-chat@kusastro.kyoto-u.ac.jp
- References: <200204050201.LAA17182@kibitaki.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
Greetings, All,
These measures of VW Hydri illustrate an interesting feature of some dwarf
novae such as VW Hydri - a distinct pause on the rise. We noticed this with
pep measures from Auckland in the 1970s and it's clearly borne out by
statistics of the visual measures. But it's good to see it so clearly
defined by Rod's measures. For what it's worth the speed through this flat
region seems directly related to the amplitude of the outburst. The UBV
measures find that the colours are quite red at this stage - B-V about 0.5
as compared with the normal negative values.
Regards,
Stan
----- Original Message -----
From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
To: <vsnet-outburst@ooruri.kusastro.kyoto-u.ac.jp>
Sent: Friday, April 05, 2002 2:01 PM
Subject: [vsnet-outburst 3787] VW Hyi brighter
> VW Hyi brighter
>
> YYYYMMDD(UT) mag observer
> 20020331.431 135 (Rod Stubbings)
> 20020401.428 <129 (Bruce Tregaskis)
> 20020401.451 137 (Rod Stubbings)
> 20020401.712 138 (Berto Monard)
> 20020404.450 130 (Rod Stubbings)
> 20020404.472 129 (Rod Stubbings)
> 20020404.496 129 (Rod Stubbings)
> 20020404.526 129 (Rod Stubbings)
>
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