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[vsnet-obs 20276] Nova suspect
- Date: Tue, 27 Apr 1999 10:46:13 -0400
- To: AAVSO <aavso@aavso.org>
- From: "W. LILLER" <wliller@compuserve.com>
- Subject: [vsnet-obs 20276] Nova suspect
- Cc: Abby Jones <afjones@voyager.co.nz>, Brian Marsden <bmarsden@CFA.Harvard.edu>, Alon Retter <ar@astro.keele.ac.uk>, VSNET <vsnet-obs@kusastro.kyoto-u.ac.jp>
- Sender: owner-vsnet-obs@kusastro.kyoto-u.ac.jp
Hi, everyone -
Here is what I am sending to Brian Marsden at CBAT:
W.Liller, Vina del Mar, Chile, writes: "A low-resolution CCD
spectrogram of Yamamoto's nova suspect obtained on Apr. 27.195 UT with a
0.20-m Schmidt camera (+ objective prism) shows H-alpha weakly in emission
approximately 20 percent brighter than the neighboring continuum,
indicating that it is a nova in the early stages of development. Its
magnitude as measured with a CCD and a broadband V filter on Apr. 27,18 was
8.45; the comparison star was the nearby B9 star SAO 186331 with Tycho V =
8.58."
All the best to all. Bill Liller
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