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[vsnet-chat 5572] Re: V 4742 Sgr
- Date: Thu, 17 Oct 2002 11:37:24 -0500
- To: aavso-discussion@informer2.cis.McMaster.CA
- From: Seiichi Yoshida <comet@aerith.net>
- Subject: [vsnet-chat 5572] Re: V 4742 Sgr
- Cc: vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp, vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@ooruri.kusastro.kyoto-u.ac.jp
Dear colleagues,
Taichi Kato wrote [vsnet-chat 5565]:
> > The star is a bona fide infrared-bright source: IRC -30347 =
> > IRAS 18001-2514 = MSX5C G005.1743-01.5120, and somewhat surprisingly is
> > also a ROSAT x-ray source 1RXS J180326.2-251556.
>
> This X-ray source is more likely associated with HD164679 (G8III/IV),
> located at 180326.4 -251558 (J2000.0). It may be noteworthy that the
> MISAO project recorded this field (MisV0502 at 180307.9 -251859).
> They may have recorded that past variability of the object(s) in question.
Unfortunately, we the MISAO Project has no images of this X-ray
object. The Image Information Search Service at:
http://vsnet.aerith.net/misao/service/info_search.html
output no images.
It is amazing because it is very near by MisV0502 as Kato-san pointed
out (thanks!). The distance between those stars is only 5 arcmin.
The position of MisV0502 was covered by KenIchi Kadota on four nights,
but MisV0502 was discovered very near by the edge of Kadota-san's
images.
Best regards,
--
Seiichi Yoshida
comet@aerith.net
http://vsnet.aerith.net/
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