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[vsnet-campaign-be 263] Re: V1294 Aql [vsnet-spectroscopy 37]
Christian's posting, quoted by Sebastian, was in regard to Delta Sco.
If my memory serves, about 15% of Be stars show "fadings" rather then
sudden outbursts.
I observed V1294 on 20030914.206 V=7.45 B-V=+0.04. V 1294 is on my
spectroscopic prgram on the coude feed at Kitt Peak. I have a run
there Sept. 30-Oct. 1.
Regards,
Thom Gandet
Petr Harmanec wrote:
>
> 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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--
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PO Box 77021
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