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[vsnet-ecl 1106] Re: [vsnet-newvar 2255] Re: New Bernhard variable (Brh V138)
- Date: Sun, 19 Oct 2003 20:41:20 -0300
- To: "Patrick Wils" <patrickwils@yahoo.com>,"Klaus Bernhard" <kl.bernhard@aon.at>,<vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp>,<dubois@simbad.u-strasbg.fr>, <gerard@simbad.u-strasbg.fr>,<samus@sai.msu.ru>, <vsnet-ecl@ooruri.kusastro.kyoto-u.ac.jp>
- From: "Sebastian Otero" <varsao@fullzero.com.ar>
- Subject: [vsnet-ecl 1106] Re: [vsnet-newvar 2255] Re: New Bernhard variable (Brh V138)
- Cc: "Peter Frank (E-Mail)" <frank.velden@t-online.de>,<herbert.raab@utanet.at>, "Chris Lloyd" <cl@ast.star.rl.ac.uk>,"Klaus Bernhard" <kl.bernhard@aon.at>,<wolfgang.moschner@t-online.de>
- Delivered-To: vsnet-ecl-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-ecl@ooruri.kusastro.kyoto-u.ac.jp
- References: <20031019230527.27833.qmail@web20803.mail.yahoo.com>
- Sender: owner-vsnet-ecl@ooruri.kusastro.kyoto-u.ac.jp
----- Original Message -----
From: "Patrick Wils" <patrickwils@yahoo.com>
> > New variable star:
> > new Brh V138 20 02 26.5 -04 46 35.4 (J2000) 13.1-14.1 (CCD)
> With the minima observed by ASAS3, the period of this star is most
> likely 1.6851 days.
> The ASAS3 data possibly also show a very shallow secondary eclipse near
> phase 0.5, but this needs confirmation.
>
> Patrick
Yes, Patrick's period is right.
I found the following elements:
Min I = HJD 2452087.723 + 1.68502 x E
V= 12.06 - 13.18
Secondary eclipse V= 12.25
Bernhard unfiltered observations were normalized to the ASAS-3 V magnitude
for the graph at:
http://ar.geocities.com/varsao/Curva_Brh_V138.htm
A very nice EA star.
Regards,
Sebastian.
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