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[vsnet-newvar 1847] SN2003aw = helium dwarf nova?
- Date: Sat, 1 Mar 2003 09:58:31 +0900 (JST)
- To: vsnet-campaign-dn@ooruri.kusastro.kyoto-u.ac.jp
- From: Taichi Kato <tkato@kusastro.kyoto-u.ac.jp>
- Subject: [vsnet-newvar 1847] SN2003aw = helium dwarf nova?
- Cc: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-newvar-archive@ooruri.kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-newvar@ooruri.kusastro.kyoto-u.ac.jp
SN2003aw = helium dwarf nova?
According to IAUC No. 8084, "SN2003aw" looks like to be a hydrogen-deficient
dwarf nova resembling KL Dra = SN1998di. The duration of the current bright
state suggests a superoutburst, if this type classification is correct.
Further observations are naturally encouraged!
(From vsnet-campaign-sn 565)
SN2003aw 20030114.0 <210C PAL
SN2003aw 20030206.26 178C PAL
SN2003aw 20030210.0 176C PAL
SN2003aw 20030219.0 178C PAL
# SN 2003aw (9:05:54.79, -05:36:08.6 (J2000.0), almost superimposed on
# the nucleus (within 2")) is hosted by also a dim galaxy.
Regards,
Taichi Kato

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