[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-alert 3267] Re: Nova Aql 99 photometry
- Date: Wed, 21 Jul 1999 16:04:18 +0200
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: Center for Backyard Astrophysics Brno station <cba@seznam.cz>
- Subject: [vsnet-alert 3267] Re: Nova Aql 99 photometry
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear dr. Retter,
many thanx for your reaction. Of course we try to make as long as possible runs but you don't know what the weather do. Yesterdays run was stoped by clouds so we went for a sleep. I'll try to make another observation and mainly spent some time on better images analyzis than yesterday. (I made only poor reduction "to see").
Could you please tell us somethink about amplitudes of changes? Or - better - is there some URL with observations of this phenomenon.
With best regards
Rudolf Novak
>Anyway, since
>typical nova periods range between ~2-10 hours
>(with a peak around
>~3.5-4 hr), a 2-hr run is usually useless
>unless spin periods of the
>rotating white dwarfs are observed. Longer runs
>and red filters are
>preferred.
-- http://email.seznam.cz
-- email zdarma na cely zivot
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp