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[vsnet-campaign-be 260] Re: [vsnet-be 141] Re: V1294 Aql [vsnet-spectroscopy 37]

Date: Sun, 14 Sep 2003 02:16:58 -0300
To: "Petr Harmanec" <hec@sunstel.asu.cas.cz>
From: "Sebastian Otero" <varsao@fullzero.com.ar>
Subject: [vsnet-campaign-be 260] Re: [vsnet-be 141] Re: V1294 Aql [vsnet-spectroscopy 37]
Cc: "Dr. Hrvoje Bozic" <hbozic@geof.hr>,"Petr Harmanec" <hec@sunstel.asu.cas.cz>,<vsnet-be@kusastro.kyoto-u.ac.jp>,<vsnet-campaign-be@kusastro.kyoto-u.ac.jp>,<vsnet-spectroscopy@ooruri.kusastro.kyoto-u.ac.jp>,"Christian Buil" <christian.buil@wanadoo.fr>
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References: <2b.45c3c9f1.2c6af248@aol.com> <000a01c36251$9af004c0$0df93251@buil> <001c01c36282$1bab7d80$2d00a8c0@168.0.1> <3F3C1CB5.AA4168A5@mindspring.com> <003a01c365f6$96fb5600$5fc43251@buil> <018201c37a74$6ba0c840$2d00a8c0@168.0.1> <Pine.LNX.4.53.0309140641080.28261@pleione.asu.cas.cz>
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>      Please, note that V1294 Aql is known to be an object with
> an inverse correlation between the brightness and emission-line strength
> already since our 1982 study (see ADS: Horn et al. 1982 BAICz 33, 308)
> and it had been observed as faint as 7.6m once in the past.

Petr, when did the star get that faint before?
I haven't seen this in the literature.

Thanks,
Sebastian.


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