[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-newvar 2255] Re: New Bernhard variable (Brh V138)
- Date: Sun, 19 Oct 2003 16:05:27 -0700 (PDT)
- To: 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
- From: Patrick Wils <patrickwils@yahoo.com>
- Subject: [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-newvar-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- In-Reply-To: <001601c39549$0c880d60$38fa2e3e@vaio>
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
> New variable star:
> new Brh V138 20 02 26.5 -04 46 35.4 (J2000) 13.1-14.1 (CCD)
>
> comments:
> Brh V138: GSC 5168 2029
> The comparison star is GSC 5168 916 (12.7 mag),
> which has been checked for constant brightness.
>
> The following observations suggest an EA variable, period still
> unknown.
> Further ASAS3 observations are available at
>
> http://vsnet.astrouw.edu.pl/~gp/asas/asas.html
>
> which confirm the variablity and the EA type.
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
__________________________________
Do you Yahoo!?
The New Yahoo! Shopping - with improved product search
http://shopping.yahoo.com
Return to Home Page
Return to the Powerful Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology