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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. --- Outgoing mail is certified Virus Free. Checked by AVG anti-virus system (http://www.grisoft.com). Version: 6.0.516 / Virus Database: 313 - Release Date: 02/09/03
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