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[vsnet-be 128] RE: [vsnet-alert 7744] Re: V1362 Cyg brightening reported by T. Ohshima



Nothing unusual on V1362 Cyg:
CYGV1362 030530.9653  8.1  DPV   7.97-3V2-8.16

Clear skies!
--------------------------------------------
Pavol A. Dubovsky & Chermelin 300/1504 mm & Binocular 12 x 60
Podbiel, SLOVAKIA - www.vkco.sk
Member of the MEDUZA group - www.meduza.info


> -----Original Message-----
> From: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
> [mailto:owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp]On Behalf
> Of Sebastian Otero
> Sent: Friday, May 30, 2003 6:05 AM
> To: vsnet-campaign-be@ooruri.kusastro.kyoto-u.ac.jp;
> vsnet-be@ooruri.kusastro.kyoto-u.ac.jp;
> vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp; Taichi Kato
> Cc: vsnet-sdor@ooruri.kusastro.kyoto-u.ac.jp;
> vsnet-campaign-sdor@ooruri.kusastro.kyoto-u.ac.jp
> Subject: [vsnet-alert 7744] Re: V1362 Cyg brightening reported by
> T. Ohshima
>
>
> It looks like a Be star with rather large amplitude variability: V= 8.09 -
> 8.23 from Hipparcos+GCPD.
> Although it's very luminous for this class.
> Anyway, one full magnitude brightening is even more than the strongest
> outburst recorded for GCAS stars (delta Sco, ome CMa, gam Cas).
> So the only thing that's left is to keep observing and confirm the event!
>
> Regards,
> Sebastian.
>
>
>
> ----- Original Message -----
> From: "Taichi Kato" <tkato@kusastro.kyoto-u.ac.jp>
> To: <vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp>;
> <vsnet-be@ooruri.kusastro.kyoto-u.ac.jp>;
> <vsnet-campaign-be@ooruri.kusastro.kyoto-u.ac.jp>
> Cc: <vsnet-campaign-sdor@ooruri.kusastro.kyoto-u.ac.jp>;
> <vsnet-sdor@ooruri.kusastro.kyoto-u.ac.jp>
> Sent: Friday, May 30, 2003 12:03 AM
> Subject: [vsnet-alert 7743] V1362 Cyg brightening reported by T. Ohshima
>
>
> > V1362 Cyg brightening reported by T. Ohshima
> >
> >   T. Ohshima-san reported that the B-type emission-line object V1362 Cyg
> > = MWC 1000 is apparently undergoing an outburst-like brightening.
> > The presently reported magnitude is about 1 mag brighter than the GCVS
> > value.  The object is known as a luminous B-type star; there may be a
> > possibility of an ongoing sudden mass-loss event.  Please see what is
> > happening!
> >
> >   YYYYMMDD(UT)   mag  code
> >   20030503.678    82  Oht.VSOLJ
> >   20030528.631    75  Oht.VSOLJ
> >   20030529.587    72: Oht.VSOLJ
> >
> > [Identifications]
> >
> > GSC2682.2966 200341.59 +362531.8 (2000.0)  8.33 1
> > 2MASS 200341.628 +362532.04 (2000.0)  7.764  7.721  7.651
> > 200341.0 +362536 (2000.0) BD+36.3841 8.0
> > 200341.4 +362532 (2000.0) HBH42-15 em V=8.1 B5II:ne
> > 200341.4 +362531 (2000.0) UBV_V1362Cyg(A) 8.15 0.17 -0.47 .030 .012 .012
> B5II:N N=4 Nm=6 *
> > 200341.5 +362532 (2000.0) SAO69334 8.2 8.3 B2
> > 200341.7 +362531 (2000.0) 190467
> > 200341.5 +362532 (2000.0) 815GV2 0.17 HIP098778 plx=1.30(0.72)
> (0.01 0.01)
> U 8.15-8.27
> > 200341.5 +362532 (2000.0) 818V
> > 200341.5 +362531 (2000.0) 819 0.10 TYC2-2682.2966.1 (8.20 0.01) (8.32
> 0.02)
> > 200341.5 +362531 (2000.0) CYGV1362 * E: 8.09 8.21 V - 7 -
> B5II:nea R1/CYG8
> > 200342.8 +362456 (2000.0) HD190467 8.0 7.8 B2
> > 200345.4 +362431 (2000.0) MWC1000 8.0 B3e
> >
> >


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