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[vsnet-newvar 1521] New Bernhard variable (Brh V120)



Dear colleagues!

I would like to send you observations of a new variable star
(Brh V120), 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 V120  184705.5 -033145.3  (J2000) 12.7-12.9 (CCD)

comments:
Brh V120:  GSC 5118  427
The comparison star is GSC 5122  294 (12.2 mag),
which has been checked for constant brightness.
The  USNO A2.0 magnitudes (r:10.8, b: 14.6) and
the following observations suggest a long period variable,
type and period still unknown.


object             YYMMDD(UT)      mag(CCD)        code
Brh V120        020626.9929            12.67            Brh.BAV
Brh V120        020628.9929            12.73            Brh.BAV
Brh V120        020705.9888            12.77            Brh.BAV
Brh V120        020707.9603            12.79            Brh.BAV
Brh V120        020708.9513            12.82            Brh.BAV
Brh V120        020719.9485            12.83            Brh.BAV
Brh V120        020814.8750            12.94            Brh.BAV
Brh V120        020814.8757            12.85            Brh.BAV
Brh V120        020814.8764            12.84            Brh.BAV
Brh V120        020814.8771            12.85            Brh.BAV
Brh V120        020814.8778            12.89            Brh.BAV
Brh V120        020814.8785            12.88            Brh.BAV


Vizier investigations show that further photometry
for this object can be found via the TASS Mk III tenxcat
database at:

http://a188-l009.rit.edu/cgi-bin/tass_curve2.cgi?281.7733_-03.5295

These observations (especially I-band) confirm the variability of GSC 5118
427.

Regards,

Klaus Bernhard

Klaus Bernhard
Kafkaweg 5
A-4030 LINZ
AUSTRIA

kl.bernhard@aon.at
http://mitglied.lycos.de/klausbernhard/

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