[vsnet-campaign-be 259] Re: V1294 Aql [vsnet-spectroscopy 37]

[Petr Harmanec <hec@sunstel.asu.cas.cz>]

Dear Colleagues,

     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.

                 Best regards,

                                                        Petr Harmanec


On Sun, 14 Sep 2003, Sebastian Otero wrote:

> Subject: Re: [vsnet-spectroscopy 37] Re: V1294 Aql
>
>
> > It's the good the interpretation of my data. The H-alpha outburst
> > is relative to the star continuum only. I have not information
> > about the magnitude evolution. Coupling spectro and
> > photometry is essential...
>
> Christian, Thom and all.
>
> V1294 Aql is at V= 7.6 so the spectral activity is confirmed in the visual.
> The range in the GCVS is V= 6.82 -7.23 but lately the star had been faint
> around 7.3-7.4.
> But never as faint as 7.6 like now. Since this is a shell Be star, a fading
> while active is what is expected so the current visual activity is in
> agreement with theory.
>
> Let's see what happens.
> Sebastian.
>
>
>
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