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[vsnet-chat 4010] Re: QX Pup
- Date: Sat, 20 Jan 2001 13:17:14 +0900
- To: CCD-astrometry-photometry@egroups.com, vsnet-chat@kusastro.kyoto-u.ac.jp
- From: Seiichiro Kiyota <skiyota@abr.affrc.go.jp>
- Subject: [vsnet-chat 4010] Re: QX Pup
- In-Reply-To: <200101191602.AA10893@runner.nofs.navy.mil>
- References: <200101191602.AA10893@runner.nofs.navy.mil>
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
In message "[vsnet-chat 4004] Re: QX Pup",aah@nofs.navy.mil wrote...
>To be strictly accurate (and less confusing!), QX Pup
>is the embedded, invisible Mira inside of the
>bipolar nebula OH 231.8+4.2.
Yes.
I don't understand yet that star like images accompany with OH 231.8+4.2 on CCD images are QX Pup (Mira variable star)
itself or bright part of planetary nebular.
I read following apaper.
Direct Detection of the Mira at the Heart of OH 231.8+4.2
Kastner, Joel H.; Weintraub, David A.; Merrill, K. M.; Gatley, Ian
The Astronomical Journal, Volume 116, Issue 3, pp. 1412-1418.
Seiichiro Kiyota
----
Seiichiro Kiyota skiyota@abr.affrc.go.jp
Laboratory of Stress Physiology
Department of Plant Physiology
National Insititute of Agrobiological Resources
Tel:81-298-38-8384
Fax:81-298-38-8347
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