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[vsnet-alert 3225] Re: possible nova in Aql
- Date: Thu, 15 Jul 1999 01:20:08 +0900 (JST)
- To: vsnet-alert@kusastro.kyoto-u.ac.jp
- From: AYANI Kazuya <ayani@bao.go.jp>
- Subject: [vsnet-alert 3225] Re: possible nova in Aql
- In-Reply-To: Your message of "Wed, 14 Jul 1999 22:41:02 +0900"<199907141339.WAA25407@mx2.nisiq.net>
- References: <199907141339.WAA25407@mx2.nisiq.net>
- Sender: owner-vsnet-alert@kusastro.kyoto-u.ac.jp
Dear vsnet members,
I have just sent a following report to CBAT.
Congraturations, Mr. Tago!
K. Ayani and T. Kawabata at Bisei Astronomical Observatory (BAO),
Okayama, Japan, obtained a low resolution spectrum (470-680nm) of the
possible nova, which was discovered by A. Tago, on July 14.6 UT with
BAO 1.01-m telescope. Strong, broad H-alpha and H-beta lines are
visible. The H-alpha line has a FWHM of about 3400 km/s and a
equivalent width of about 50 nm.
Best regards,
Kazuya Ayani
Bisei Astronomical Observatory
Return to Daisaku Nogami
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