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[vsolj-alert 516] SN1999gq
- Date: Tue, 28 Dec 1999 23:04:53 +0900 (JST)
- To: vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsolj-alert 516] SN1999gq
- Sender: owner-vsolj-alert@ooruri.kusastro.kyoto-u.ac.jp
From owner-vsnet-alert@kusastro.kyoto-u.ac.jp Tue Dec 28 01:34 JST 1999
To: isn_chat@supernovae.net, vsnet-alert@kusastro.kyoto-u.ac.jp
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Date: Tue, 28 Dec 1999 01:05:25 +0900 (JST)
From: AYANI Kazuya <ayani@bao.go.jp>
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Subject: [vsnet-alert 3862] Spectroscopy of SN 1999gq
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Spectroscopy of SN 1999gq
Dear colleagues,
I have posted the following report to CBAT.
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SUPERNOVA 1999gq IN NGC 4523
K. Ayani, Bisei Astronomical Observatory (BAO), and H. Yamaoka,
Kyushu University, report: "We obtained a wide-band spectrum (range
400-800 nm; resolution 0.6 nm) of SN 1999gq with the BAO 1.01-m
reflecter on Dec. 26.84 UT. It shows that the supernova is of type-II
in the early phase, with a broad P-Cyg H-alpha profile and H-beta
absorption on a blue continuum. Adopting the NED recession velocity
for NGC 4523 (260 km/s), the expansion velocity of the supernova,
derived from H-alpha absorption minimum, is 7800 km/s. Other broad
absorption features are seen at 580, 559, 510, 495 nm on the rest
frame of the host galaxy."
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Best regards,
Kazuya Ayani
Bisei Astronomical Observatory
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