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[vsnet-chat 2077] Re: BV sequence for V1333 Aql



Re: [vsnet-chat 2074] BV sequence for V1333 Aql

>      The GCVS4.1 claims a peak magnitude of 14.8, so perhaps it is readily
> accessible only to those with large telescopes (or smaller ones + CCD).

   The quoted GCVS maximum seems to be a rather exceptional value.  Recent
reports (cf. IAUCs) indicate usual optical maxima are around mag 16.  At
the time of charting, it did look readily accessible, since several 14.5-15.0
mag dwarf novae were already on the program (as are reported in VSNET now).
Aside from usual outbursts, there was a report (in ApJ letter, last year?)
of recurrent short optical flashes.  I wonder whether this phenomenon has
been confirmed, and whether is accesible to eyes.

Regards,
Taichi Kato

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