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[vsnet-obs 24340] New variable (BeV30)
- Date: Sat, 30 Oct 99 06:39:57 PDT
- To: vsnet-obs@kusastro.kyoto-u.ac.jp, dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.su
- From: "Klaus Bernhard" <klaus.bernhard@vpn.at>
- Subject: [vsnet-obs 24340] New variable (BeV30)
- Cc: herbert.raab@ris.at, "Chris Lloyd" <cl@astro1.bnsc.rl.ac.uk>, "Mike Collins" <101763.3365@compuserve.com>, "Wolfgang Moschner" <wolfgang.moschner@t-online.de>
- Priority: Normal
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Dear colleagues!
I would like to send you observations of a new variable star (BeV30),
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 BeV30 233232.6 N103320 (J2000) 12.1 12.4(CCD)
comments:
BeV30: GSC 1172 1452
Comparison star was for all measurements GSC 1172 1385 (11.7 mag),
which was checked to be constant.
Data analysis was made by Chris Lloyd, UK. His comment:
Strong series of periods increasing towards higher frequency. The
best period is 0.2065 days so it may be a beta Cep or delta Sct, or
something similar.
object YYMMDD(UT) mag (CCD) code
BeV30 990911.0056 12.19 BRH.BAV
BeV30 990911.9972 12.22 BRH.BAV
BeV30 990912.9979 12.28 BRH.BAV
BeV30 990913.9896 12.42 BRH.BAV
BeV30 990915.0201 12.40 BRH.BAV
BeV30 990923.9632 12.28 BRH.BAV
BeV30 990927.9556 12.20 BRH.BAV
BeV30 991002.0451 12.12 BRH.BAV
BeV30 991007.9291 12.43 BRH.BAV
Regards,
Klaus Bernhard
Klaus Bernhard
Kafkaweg 5
A-4030 LINZ
AUSTRIA
e-mail:
klaus.bernhard@vpn.at
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