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[vsnet-chat 4575] Re: HD 235749 (was Re: new Tycho variables...)
- Date: Sun, 1 Jul 2001 01:44:29 -0300
- To: "Taichi Kato" <tkato@kusastro.kyoto-u.ac.jp>, <vsnet-chat@kusastro.kyoto-u.ac.jp>, <vsnet-newvar@kusastro.kyoto-u.ac.jp>
- From: "Sebastian Otero" <varsao@sinectis.com.ar>
- Subject: [vsnet-chat 4575] Re: HD 235749 (was Re: new Tycho variables...)
- References: <200107010204.LAA28680@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
> > HD 235749 / 8.81, 1.71 ; 8.93, 1.60
> > This one seems to be an ordinary red variable deserving attention !!!
>
> Not an ordinary red variable! The star has a composite spectrum
> of OB+M (according to the LS catalog), and is cataloged as an emission
> line object. VV Cep-type? Symbiotic-like object?
>
> The object has a NSV name: NSV25855 (9.01-9.30V). Those who are
> going to make observing reports on this object are strongly recommended
> to use this designation.
>
> Regards,
> Taichi Kato
Very interesting!
I didn't make any identification but to search for photometry !!
In spite of the faint NSV range, PEP(V) magnitudes and even Tycho 2
magnitude (V= 8.91) are brighter.
Actually the star is included in a list of VV Cep-type stars observed
photometrically in Miroscnichenko and Ivanov, 1993, from which the NSV
magnitudes comes from. The color of the star was measured between 1.57 and
1.76 (B-V).
But the star was first classified as VV Cep by Barbier as early as 1971.
So the amplitude is greater than catalogued: 8.8 - 9.3 V at least.
Regards,
Sebastian.
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