> 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. --- 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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