[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-newvar 2017] Re: New Bernhard variable (Brh V134)
- Date: Thu, 19 Jun 2003 17:34:15 +0100 (BST)
- To: Klaus Bernhard <kl.bernhard@aon.at>
- From: Chris Lloyd <cl@astro1.bnsc.rl.ac.uk>
- Subject: [vsnet-newvar 2017] Re: New Bernhard variable (Brh V134)
- Cc: <samus@sai.msu.ru>, <vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp>,Wolfgang Quester <WQUESTER@aol.com>,Wolfgang Moschner <wolfgang.moschner@t-online.de>,<herbert.raab@utanet.at>,"Peter Frank (E-Mail)" <frank.velden@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: <002201c3359c$09d79700$1ef92e3e@vaio>
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
Dear All,
By combining Bernhard's data of BeV134 with that from ASAS3 I think the
star is a convincing W UMa variable. The preliminary ephemeris is
JD_minI = 2452025.63 + 0.24207xE
The variable has a full amplitude of 0.6 mag which suggests that it is a
high-inclination system, although neither of the eclipses look total.
Cheers,
Chris
Return to Home Page
Return to the Powerful Daisaku
vsnet-adm@kusastro.kyoto-u.ac.jp
Powered by ooruri technology