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[vsnet-id 755] V1485 Cyg = NSV 12235
- Date: Sun, 2 Mar 2003 00:04:42 -0700 (MST)
- To: vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- From: Brian Skiff <Brian.Skiff@lowell.edu>
- Subject: [vsnet-id 755] V1485 Cyg = NSV 12235
- Delivered-To: vsnet-id-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-id@ooruri.kusastro.kyoto-u.ac.jp
As best I can tell, comparing the finder charts for these two stars
appearing in 1906AN....172..349W and in 1974VatOP...1..181C, they are
identical, despite their conflicting variability types. The star is
a red IRAS source, so the semiregular type is certain (the NSV star is
suspected of being an Algol-type eclipser).
\Brian
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