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[vsnet-chat 1259] Re: H/T chart vs. VT mags...
- Date: Thu, 03 Sep 1998 01:47:04 +0930
- To: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- From: "Fraser Farrell" <fraserf@dove.net.au>
- Subject: [vsnet-chat 1259] Re: H/T chart vs. VT mags...
- CC: vsnet-chat@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
G'day all,
> and even +0.5(B-V). From my experience and estimates of other observers
> in my country, such large positive term is incredible. Perhaps Japanese
> observers are red-sentive (less adapted to catacluysmics ;-), or they too
> suffer from the light pollution to fully attain dark adaptation...
My guess would be light pollution. I have noticed on many occasions how
a starfield being observed will suddenly change character when my local
football club finally turns off its floodlights! There is a similar
(but slower) effect when the Moon rises or sets.
Perhaps the equation should read :
(visual mag) = V + 0.2(B-V) + (streetlight density factor) ? ;-)
> I have heard comet observers use VT rather than V. I would love to hear
> comments from them also.
I know that Bill Bradfield uses V mags (from a variety of printed
sources), because he doesn't have access to VT mags (or a computer).
Justin Tilbrook works from the closest variable star sequence (usually V
or SPv from VSS RASNZ). I still use V to maintain consistency with my
historical estimates.
cheers,
Fraser Farrell
http://vsnet.dove.net.au/~fraserf/ email: fraserf@dove.net.au
traditional: PO Box 332, Christies Beach, SA 5165, Australia
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