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[vsolj-alert 87] V893 Sco is a real UG star!

From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Sat Apr 18 18:59 JST 1998
Date: Sat, 18 Apr 1998 18:57:27 +0900 (JST)
From: Daisaku Nogami <nogami>
To: vsnet-alert
X-Distribute: distribute [version 2.1 (Alpha) patchlevel=24]
Subject: [vsnet-alert 1688] The dwarf nova nature of V893 Sco
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Dear colleagues,

We made spectroscopic observations of V893 Sco just recently
rediscovered by Kato et al. (submitted to IBVS) by the NTT
telescope at ESO on April 18.4 (UT).  Then, we confirmed the
dwarf novae nature of this star by detecting double-peaked
strong emmision lines of Halpha and Hbeta, suggesting V893 Sco
to be a high-inclination system.

Best regards,
Daisaku Nogami, Ronald Mennickent, and Katsura Matsumoto

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