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[vsnet-mira 62861] Re: [vsnet-newvar 267] New Takamizawa variable (TmzV716)
- Date: Mon, 28 Feb 2000 11:32:34 +0000 (GMT)
- To: vsnet-mira@kusastro.kyoto-u.ac.jp, Kesao Takamizawa <GHA07243@niftyserve.or.jp>
- From: Chris Lloyd <cl@ast.star.rl.ac.uk>
- Subject: [vsnet-mira 62861] Re: [vsnet-newvar 267] New Takamizawa variable (TmzV716)
- cc: dubois@simbad.u-strasbg.fr, gerard@simbad.u-strasbg.fr, samus@sai.msu.ru, vsnet-newvar@kusastro.kyoto-u.ac.jp
- In-Reply-To: <200002271102.UAA11670@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-mira@kusastro.kyoto-u.ac.jp
A period analysis of the observations of TmzV716 recently reported by
Takamizawa suggest that the star is a Mira with an amplitude of at least
5 magnitudes and a well determined period of 310 days. The ephemeris of
maximum light is
JD_max = 2451594.0 + 310.0xE
The light curve is smooth but quite asymmetric, and the star is currently
just after maximum light.
Regards Chris Lloyd