[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-chat 4012] Re: QX Pup
- Date: Sat, 20 Jan 2001 17:59:43 +0900 (JST)
- To: CCD-astrometry-photometry@egroups.com
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 4012] Re: QX Pup
- Cc: vsnet-chat, vsnet-lpv
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: QX Pup
> If the starlight were not entirely visible, how come the spectral
> classification of M6I or M9III was obtained ?? Are we observing the
> scattered light from the Mira star?
For example, A&A 355, 1103 (2000), clearly shows the M-type spectrum
in the optical, indicating the presence of significant amount of scattered
starlight contributing to the optical light.
Regards,
Taichi Kato
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp
VSNET Home Page