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[vsnet-chat 47] Re: supernova progenitor candidates
- Date: Mon, 10 Feb 1997 23:43:02 +0900 (JST)
- To: vsnet-chat
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-chat 47] Re: supernova progenitor candidates
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Yamaoka Hitoshi wrote:
> I guess that the best candidate among the brightest (m_v < 2.5) stars
> is Betelgeuse, but the time of the explosion event is not certain: it
> can be today, but it can also be after about a million years.
Encouraged to hear this! This star then well deserves observer's
nightly visit -- as well as other SRc variables. If one can visit 1000
SRc variables, there may be a chance to catch a supernova explosion in
1000 years -- am I right? I wonder what the progenitor of the Crab nebula
or Tycho's star would have been like -- was it a naked-eye star?
How about LMC/SMC stars? Is there any systematic monitoring program?
What target selection? How about the Orion Nebula stars?
> From the table of the binaries in _Chronological Scientific Tables
> (Rika Nenpyo, Japan)_, 32 Cyg A is K1I supergiant and has 23 solar
> mass. It should be doubtless to say that it will go supernova next
> one million years.
Thank you! I will add this star to my visual monitoring program <g>.
Hoping the exposion is detected before the binary is engulfed by the blast.
Regards,
Taichi Kato
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