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[vsnet-newvar 766] New Bernhard variable (Brh V66)
- Date: Sun, 25 Feb 2001 18:36:43 -0800
- To: "dubois@simbad.u-strasbg.fr" <dubois@simbad.u-strasbg.fr>, "gerard@simbad.u-strasbg.fr" <gerard@simbad.u-strasbg.fr>, "samus@sai.msu.ru" <samus@sai.msu.ru>, "vsnet-newvar@kusastro.kyoto-u.ac.jp" <vsnet-newvar@kusastro.kyoto-u.ac.jp>, "frank.velden@t-online.de" <frank.velden@t-online.de>
- From: Klaus Bernhard <kl.bernhard@aon.at>
- Subject: [vsnet-newvar 766] New Bernhard variable (Brh V66)
- CC: Wolfgang Moschner <wolfgang.moschner@t-online.de>, Herbert Raab <herbert.raab@ris.at>, Chris Lloyd <cl@astro1.bnsc.rl.ac.uk>, "101763.3365@compuserve.com" <101763.3365@compuserve.com>, Andreas Berthold <andreas.berthold@chello.at>, "kpo.v" <gorlin@telia.com>
- Sender: owner-vsnet-newvar@kusastro.kyoto-u.ac.jp
Dear colleagues!
I would like to send you observations of a new variable star (Brh V66),
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 V66 061542.4 +162813 (J2000) 11.6 12.3 (CCD) SR
comments:
Brh V66: GSC 1314 1193
Comparison star was for all measurements GSC 1314 8 (11.9 mag),
which was checked to be constant.
The apparently slow change in brightness and the red colour
(USNO A2.0 r:12.1, b: 16.4) suggest a SR-variable.
object YYMMDD(UT) mag (CCD) code
Brh V66 001221.0153 11.66 Brh.BAV
Brh V66 001222.9875 11.64 Brh.BAV
Brh V66 001223.9813 11.55 Brh.BAV
Brh V66 010114.9153 12.06 Brh.BAV
Brh V66 010116.0174 12.09 Brh.BAV
Brh V66 010118.9125 11.99 Brh.BAV
Brh V66 010128.0063 12.25 Brh.BAV
Brh V66 010224.8479 11.66 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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