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[vsnet-chat 444] PG1136+581 ...
- Date: Thu, 17 Jul 1997 15:36:09 -0400
- To: vsnet-chat@kusastro.kyoto-u.ac.jp
- From: "John R. Thorstensen" <thorsten@Dartmouth.EDU>
- Subject: [vsnet-chat 444] PG1136+581 ...
- Sender: owner-vsnet-chat@kusastro.kyoto-u.ac.jp
Colleagues,
This object is definitely an emission line galaxy.
Its spectrum shows strong, narrow nebular lines at a
small redshift.
Incidentally, I have recently obtained spectra of
another tentative CV in the D&S catalog, Peg5 =
KUV23182+1007. It proves to be a QSO at a redshift of
0.66. At this redshift, MgII 2800 redshifts to near
HeII 4686, which confused the original investigators.
Farther to the red it shows narrow [OII] 3727 at the
correct redshift, which clinches the identification.
So it moves from "cv:" to definitely "non-cv".
John Thorstensen
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