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[vsnet-alert 5138] Delta Sco: a new extremely bright Gamma Cas-type star in outburst
- Date: Fri, 21 Jul 2000 23:01:45 +0900 (JST)
- To: vsnet-alert
- From: Taichi Kato <tkato>
- Subject: [vsnet-alert 5138] Delta Sco: a new extremely bright Gamma Cas-type star in outburst
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Delta Sco: a new extremely bright Gamma Cas-type star in outburst
The following messages are from Sebastian Otero. Delta Sco has now
become one of the brightest gamma Cas stars (active Be stars) among
historically recorded outbursts of this class. The phenomenon is apparently
ongoing, and the object may attain the 1-st magnitude brightness.
Please watch closely and report your observations!
Subject: [vsnet-be 2] (fwd) Delta Sco - GCAS???
The bright B0.5IV star DELTA SCORPII is probably brighter than normal.
It looks like 2.2 instead of 2.3.
I searched for photometric data in the past and there are several
measurements in the range 2.31 - 2.33. But there is one isolate 2.21
(Hogg A.R., 1958, "Photometric observations of 244 bright stars") that
makes me suspicious. It's been some weeks since I noticed this probable
little brightening but I hadn't paid much attention. In addition, the
Hipparcos Catalogue gives a brighter value of 2.29.
Several suitable comparison stars may be used in estimating:
GAMMA CEN: 2.16
ALPHA LUP and EPSILON CEN: ~2.30*
KAPPA SCO: 2.40*
ETA OPH: 2.43
(These 3 stars are BCEP variables but the amplitude is very small)
Of course, the variability is too small for being followed visually, but
it would be interesting to do some photometry in order to confirm this
probable brightening. Could it be a possible GCAS variable? The
behaviour is similar to that of ALPHA ARAE and ETA CENTAURI. Could a new
spectrum taken right now show emission lines?
I hope someone can measure it. I just have my eyes...
Sebastian Otero.
Subject: [vsnet-be 3] SPECTROSCOPIC CONFIRMATION of Delta Scorpii variability
WE HAVE A NEW VARIABLE STAR CONFIRMED.
And it's one of the brightest.
Spectroscopic observations show that the H Alpha line is in emission.
DELTA SCORPII IS A NEW GCAS star.
This confirmation came from Spain and it will be reported to the IAU.
Sebastian Otero.
Recent observations:
YYYYMMDD(UT) mag observer
20000626.901 22 (S. Otero)
20000630.028 22 (S. Otero)
20000704.078 22 (S. Otero)
20000716.928 21 (S. Otero)
20000717.123 21 (S. Otero)
20000718.949 21 (S. Otero)
20000720.018 20 (S. Otero)
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