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[vsnet-newvar 1459] re CGCS 1749
- Date: Tue, 11 Jun 2002 17:09:55 +0000
- To: vsnet-newvar@kusastro.kyoto-u.ac.jp
- From: jg <jg@jgws.freeisp.co.uk>
- Subject: [vsnet-newvar 1459] re CGCS 1749
- Delivered-To: vsnet-newvar@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
With regards to CGCS 1749
(http://vsnet.kusastro.kyoto-u.ac.jp/vsnet/Mail/vsnet-newvar/msg01458.html)
being possibly more variable the bluer you look, and virtually constant
in the far-red.
Could anyone with experience comment on this with respect to the
behaviour of RCB stars, thinking generally with respect to their
non-fading states?
I'm only picking up general throw-away comments from books and online
literature searches for articles aren't going too well either.
Thanks
John
John Greaves
UK
Return to Daisaku Nogami
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