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[vsnet-chat 4101] Re: [vsnet-campaign 772] SN1989Z
- Date: Mon, 19 Feb 2001 22:10:04 +0100
- To: vsnet-campaign@kusastro.kyoto-u.ac.jp, vsnet-chat@kusastro.kyoto-u.ac.jp, vsnet-gcvs@kusastro.kyoto-u.ac.jp
- From: Patrick Schmeer <extpasc@rz.uni-sb.de>
- Subject: [vsnet-chat 4101] Re: [vsnet-campaign 772] SN1989Z
- In-Reply-To: <200102191312.WAA05764@ceres.kusastro.kyoto-u.ac.jp>; from tkato@kusastro.kyoto-u.ac.jp on Mon, Feb 19, 2001 at 10:12:39PM +0900
- References: <200102191312.WAA05764@ceres.kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
The alleged Supernova 1989Z (= EQ J1158+4356) is merely a constant foreground
star of NGC 4013 (cf. IAUC 6911, 6914, 6920).
Regards,
Patrick
On Mon, Feb 19, 2001 at 10:12:39PM +0900, Taichi Kato wrote:
> SN1989Z
>
> According to the latest version of CV Catalog (Downes et al.), the
> following object is listed as a possible CV.
>
> 115832.0 +435658 (2000.0) SN1989Z G N4013 10E 4N - - - M.Shaw
>
> According to the catalog, the range is listed as 12.5V - 17.
>
> The apparent "host" galaxy is not a remote one, but the "SN" may have been
> regarded as a foreground cataclysmic variable based on other reasons.
> The object is not listed in GCVS/NSV.
>
> Monitoring for future outbursts are strongly recommended.
>
> Please report the object with the name SN1989Z.
>
> Regards,
> Taichi Kato
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