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[vsnet-alert 7516] SN Ia 2002fk
- Date: Sun, 22 Sep 2002 01:12:48 +0900 (JST)
- To: vsnet-campaign-sn@kusastro.kyoto-u.ac.jp, vsnet-alert@kusastro.kyoto-u.ac.jp, isnchat@yahoogroups.com
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-alert 7516] SN Ia 2002fk
- Delivered-To: vsnet-alert@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
Dear SN watchers,
In [vsnet-alert 7494]:
> The reported magnitudes suggest that it is in a rising phase.
>Typical SN Ia at maximum would be mag about 14.1 for this galaxy.
>Follow-up photometry and spectroscopic classification is urged.
Spectroscopy at Bisei confirmed that SN 2002fk is really of type Ia.
Following is a report submitted to IAU circular.
SUPERNOVA 2002fk in NGC 1309
K. Ayani, Bisei Astronomical Observatory (BAO) and H. Yamaoka,
Kyushu University, write: "A low-resolution spectrum (range 500-700
nm) of SN 2002fk (IAUC 7973), obtained with BAO 1.01-m telescope on
Sept. 20.7 UT, indicates that it is a type-Ia supernova before
maximum light. Adopting the NASA/IPAC Extragalactic Database
recession velocity of 2135 km/s, the expansion velocity deduced from
Si II (rest 635.5 nm) is about 10900 km/s.
Sincerely Yours,
Hitoshi Yamaoka, Kyushu Univ., Japan
yamaoka@rc.kyushu-u.ac.jp
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