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[vsnet-chat 1605] Re: V491 Car
- Date: Thu, 4 Feb 1999 16:22:57 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato>
- Subject: [vsnet-chat 1605] Re: V491 Car
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Re: [vsnet-chat 1602] V491 Car
> Probably eclipsing system??
The spectrum is K3V. Assuming an eclipsing system, this spectrum should
be of the primary. In this case the observed amplitude (>3 mag) seems to
be to large, unless we consider a black dwarf secondary ;-) having a similar
size of a K3V star.
Regards,
Taichi Kato
Return to Daisaku Nogami
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