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[vsnet-campaign-sn 639] SN II 2003gd in M 74
- Date: Mon, 16 Jun 2003 14:26:14 +0100
- To: vsnet-campaign-sn@kusastro.kyoto-u.ac.jp
- From: lblopes@ncc.up.pt
- Subject: [vsnet-campaign-sn 639] SN II 2003gd in M 74
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- In-Reply-To: <200306140514.h5E5EVr7004401@rcsvr.rc.kyushu-u.ac.jp>
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Quoting Hitoshi YAMAOKA <yamaoka@rc.kyushu-u.ac.jp>:
> The first spectrum was taken on the same night at America, i.e. June
> 13.46 UT = 0.64 days after discovery. The IR spectrum shows a series
> of strong and broad hydrogen Paschen emission lines, which indicates
> that is it a type II SN around maximum.
Is there any indication so far on whether this SN is still on the rise ?
I imagine the strong, broad, IR hydrogen lines observed point to the
possibility that the star was caught shortly after the collapse, right ?
Best,
Luis Lopes
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