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[vsnet-newvar 1032] New Bernhard variable (Brh V93)



Dear colleagues!

I would like to send you observations of a new variable star (Brh V93),
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 V93 182203.3 +072137  (J2000) 12.7-13.0 (CCD) SR

comments:
Brh V93: GSC 444 2502
The comparison star is GSC 444 2300  (12.3 mag),
which has been checked for constant brightness.
The colour (USNO A2.0 r: 11.8, b: 14.2) and the apparently 
slow change of brightness suggest a SR-variable. 
Other types of variability cannot be excluded.

object          YYMMDD(UT)    mag (CCD)   code

Brh V93		010625.0014	12.86	Brh.BAV
Brh V93		010625.9674	12.80	Brh.BAV
Brh V93		010626.9660	12.93	Brh.BAV
Brh V93		010705.9576	12.95	Brh.BAV
Brh V93		010709.9611	12.80	Brh.BAV
Brh V93		010714.9688	12.74	Brh.BAV
Brh V93		010715.9417	12.67	Brh.BAV
Brh V93		010717.9556	12.68	Brh.BAV
Brh V93		010721.9472	12.65	Brh.BAV
Brh V93		010728.9444	12.73	Brh.BAV
Brh V93		010730.9521	12.81	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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