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[vsnet-newvar 940] New Bernhard variable (Brh V75)



Dear colleagues!

I would like to send you observations of a new variable star (Brh V75),
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 V75 170222.6 +041027  (J2000) 11.0 11.4 (CCD) SR?

comments:
Brh V75: GSC 406 1063
The comparison star is GSC 406 887  (12.1 mag),
which has been checked for constant brightness.
The apparently slow change of brightness suggests
a SR-variable. 
The USNO A2.0 magnitudes (r: 10.9, b: 13.2) have the remark
"magnitudes are probably wrong".


object          YYMMDD(UT)    mag (CCD)   code

Brh V75         000702.8957	11.12	Brh.BAV	
Brh V75         000706.8971	11.06	Brh.BAV
Brh V75         000717.8735	11.03	Brh.BAV
Brh V75         000720.8714	11.00	Brh.BAV
Brh V75         000731.8707	11.15	Brh.BAV
Brh V75         000801.8658	11.13	Brh.BAV
Brh V75         000809.8804	11.29	Brh.BAV
Brh V75         000811.8450	11.33	Brh.BAV
Brh V75         000812.8499	11.29	Brh.BAV
Brh V75         000814.8471	11.32	Brh.BAV
Brh V75         000816.8401	11.35	Brh.BAV
Brh V75         000819.8374	11.33	Brh.BAV
Brh V75         000820.8401	11.28	Brh.BAV
Brh V75         010614.9457	11.36	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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