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[vsnet-be 45] Re: Omega CMa comparison stars
- Date: Thu, 19 Apr 2001 12:40:05 +0900 (JST)
- To: vsnet-be, vsnet-campaign-be, vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-be 45] Re: Omega CMa comparison stars
- Sender: owner-vsnet-be@kusastro.kyoto-u.ac.jp
Re: Omega CMa comparison stars
> It is important to say that one should be careful in using them, but I think
> care must be taken in every estimate we make (see vsnet-chat 4199 and 4233).
> Every time I estimate a variable, it's like estimating its comparisons since
> I take the job of checking if everything is "okay". Using similar comparions
> (eg= 3.82, 3.96, 4.20), any difference between them would be perceived and
> .... and then I would send an alert !!!!
I think that this is the best approach for visual photometry -- the use
of an emsemble of stars when a set of comparison stars unavoidably include
possible microvariables. The same situation is met in bright Cassiopeia
variables in the northern hemisphere (almost all stars are suspected of
variability).
Nevertheless, 3 Pup deserves more attention because it's one of
"prototype" stars of these high-luminosity peculiar stars. They may be
variable in a large amplitude, and individual observations may be worth
reporting even when the star is quiet.
Regards,
Taichi Kato
vsnet-adm@kusastro.kyoto-u.ac.jp
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