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[vsnet-obs 38578] Re: [vsnet-chat 5109] Re: Magnitude p of variable stars
- Date: Thu, 21 Feb 2002 05:28:00 EST
- To: tkato@kusastro.kyoto-u.ac.jp, toniscarmato@hotmail.com, vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp, vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
- From: Pete1199@aol.com
- Subject: [vsnet-obs 38578] Re: [vsnet-chat 5109] Re: Magnitude p of variable stars
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
In a message dated 2/20/02 11:55:06 PM Eastern Standard Time,
tkato@kusastro.kyoto-u.ac.jp writes:
<< > The catalog incluse in Megastar Program 4.0 is the GCVS.
> This catalog is not reliable? >>
The problem is probably due to the fact that often the positions given by the
discover are incorrect. Variables discovered on photographic plates often are
misidentified. Some of the discovery charts are quite confusing. Brian Skiff
has published a number of IBVS issues which give the correct location of some
of these stars.
... PG
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