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[vsnet-chat 1320] Re: Host galaxy of SN 1998eb
- Date: Sun, 20 Sep 1998 00:37:40 -0700
- To: tkato@kusastro.kyoto-u.ac.jp
- From: bas@lowell.Lowell.Edu (Brian Skiff)
- Subject: [vsnet-chat 1320] Re: Host galaxy of SN 1998eb
- Cc: isn_chat@mbox.queen.it, vsnet-chat@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
> IRAS05365+6921 053633.0 +692101 (1950.0)
> F12=0.52 F25=0.48 F60=6.31 F100=22.90
> VAR= 6 LRS=-1
> VIb: variable star with relatively hot dust close to
> the star and relatively cold dust at large distance
> may be O-rich
...obviously the IRAS spectral "classifications" can be misleading.
The IRAS sources that peak at 60 or 100 microns can be just about any sort
of "nebula": reflection, emission, circumstellar shell, planetary nebula,
or a galaxy.
\Brian
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