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[vsnet-alert 7020] (fwd) More on IM Nor
- Date: Sun, 13 Jan 2002 11:12:32 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp, vsnet-campaign-nova@ooruri.kusastro.kyoto-u.ac.jp, vsnet-discovery-nova@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-alert 7020] (fwd) More on IM Nor
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
(fwd) More on IM Nor
Date: Sat, 12 Jan 2002 13:02:13 -0500
From: "W.Liller" <wliller@compuserve.com>
Subject: More on IM Nor
Hola again -
Last night, Jan.12.330 UT, using a CCD and a 20cm f/1.5 Schmidt camera, I
measured the position of the recurrent nova to be (2000) RA = 15h 39m
26.61s +/- 0.18s, Dec. -52d 19' 18.6" +/- 0.5". This agrees moderately
well with the position for IM Normae measured from a Harvard MC plate: end
figures: 26.26s, 21.4" (See Duerbeck, A Reference Catalogue and Atlas of
Galactic Novae. Reidel, 1987).
The magnitude, measured from the same CCD frame and with a minus-red-and-IR
filter -- I call it V(bv) = was 8.13 +/- 0.03. The comparison stars used
were GSC 8308 511 and 8308 651.
A low-dispersion objective prism spectrum, taken Jan. 12.351 UT, shows
H-alpha to be very strong and relatively narrow with FWHM = 950 km/sec
+/-50. Other lines of the Balmer Series, the Fe II multiplets 42 and 74,
and O I at 777.1 nm are also clearly present.
All the best to all, Bill Liller
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