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[vsnet-obs 42244] SN observations from IAUC 8011-12
- Date: Sat, 9 Nov 2002 12:05:08 +0900 (JST)
- To: vsnet-obs@kusastro.kyoto-u.ac.jp
- From: Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>
- Subject: [vsnet-obs 42244] SN observations from IAUC 8011-12
- Cc: vsnet-campaign-sn@kusastro.kyoto-u.ac.jp
- Delivered-To: vsnet-obs@kusastro.kyoto-u.ac.jp
- Sender: owner-vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
SN2002ho 20020403.0 <185C Bol
SN2002ho 20021105.130 170C Bol
SN2002ho 20021107.528 168C SCH
# NGC 4210, a host galaxy of SN 2002ho (12:15:17.97 +65:58:55.1
# (J2000.0), offset = 13"E, 12"S), is a barred-spiral (SB(r)b) galaxy.
# SN is superimposed on the southern arm. Typical SN Ia in this
# galaxy would have a maximum of mag about 14.5, but it seems not the
# case for this SN.
# SNe 2002hp-ht were discovered by the HST.
SN2002hu 20021004.0 <185C Bol
SN2002hu 20021107.09 170C Bol
# MCG +06-6-12 = KUG 0215+372, a host galaxy of SN 2002hu (2:18:20.06,
# +37:27:58.8 (J2000.0), offset = 21"E, 7"N), is a small spiral galaxy
# with ultraviolet excess.
SN2002hv 20020428.2 <190:C KAI
SN2002hv 20021105.5 186C SCH
SN2002hv 20021107.5 189:C SCH
# UGC 4974, a host galaxy of SN 2002hv (9:22:10.91, +33:50:10.8
# (J2000.0), offset = 7"E, 43"S), is a lenticular (S0:) galaxy making
# a pair with KUG 0919+340. Such early (E-S0) galaxies produce SN Ia
# only, whose expected maximum is mag about 16.5. It is probably old
# SN Ia.
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