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[vsnet-newvar 1037] New Bernhard variable (Brh V95)



Dear colleagues!

I would like to send you observations of a new variable star (Brh V95),
which I have discovered in a systematic CCD-based search for new
variables.
In each observing run typically 400 images are taken of several survey
fields.
The frames are processed automatically.

Instruments:
CCD-camera: Starlight Xpress SX (unfiltered)
Telescope: Celestron-8 (20 cm Schmidt-Cassegrain)

New variable star:
new Brh V95 184110.9 +071451  (J2000) 12.2-12.4 (CCD) SR

comments:
Brh V95: GSC 459 621
The comparison star is GSC 459 397  (12.1 mag),
which has been checked for constant brightness.
The colour (USNO A2.0 r: 12.0, b: 15.2) and the apparently 
slow change of brightness suggest a SR-variable
with a period of about 40 days. 
Other types of variability cannot be excluded.

object          YYMMDD(UT)    mag (CCD)   code
Brh V95		010625.0142	12.18	Brh.BAV
Brh V95		010625.9801	12.17	Brh.BAV
Brh V95		010626.9788	12.17	Brh.BAV
Brh V95		010703.9614	12.21	Brh.BAV
Brh V95		010704.9669	12.18	Brh.BAV
Brh V95		010705.9704	12.22	Brh.BAV
Brh V95		010709.9739	12.26	Brh.BAV
Brh V95		010714.9815	12.36	Brh.BAV
Brh V95		010715.9544	12.41	Brh.BAV
Brh V95		010717.9683	12.35	Brh.BAV
Brh V95		010721.9600	12.31	Brh.BAV
Brh V95		010722.9572	12.35	Brh.BAV
Brh V95		010728.9572	12.24	Brh.BAV
Brh V95		010730.9649	12.17	Brh.BAV

Regards,

Klaus Bernhard

Klaus Bernhard
Kafkaweg 5
A-4030 LINZ
AUSTRIA

kl.bernhard@aon.at
http://mitglied.tripod.de/KlausBernhard/index.html

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