[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 4005] Re: QX Pup
- Date: Sat, 20 Jan 2001 01:29:47 +0900 (JST)
- To: CCD-astrometry-photometry@egroups.com
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 4005] Re: QX Pup
- Cc: vsnet-chat, vsnet-lpv
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: QX Pup
> To be strictly accurate (and less confusing!), QX Pup
> is the embedded, invisible Mira inside of the
> bipolar nebula OH 231.8+4.2.
The light of the Mira star is already visible in the J-band (as the GCVS
tells). I won't wonder if detectable Mira-type variability is recorded
in the I-band (observable with conventinal CCDs).
There are a variety of stars at this or the following evolutionary stage,
some of which visible to human eyes compose favorite targets of variable
star observers.
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp