摘要
据观测到的ＳＮ１９９６的Ｈα谱线的初步计算结果表明，该超新星可能是由一颗晚Ｂ９型超新星爆发形成的，爆发时的气壳质量可达０．００３１Ｍ⊙，径向膨胀速度为１１７６０ｋｍ／ｓ。
おhe preliminary analysis of Hα profile for SN1996w is presented in this paper.It is shown that SN1996w may be formed by a B9 super giant expoloded.It has a shell with the mass of 0.0031 M⊙ and the radial expanding velocity of about 11760km/s.
出处
《云南天文台台刊》
CSCD
1998年第2期8-14,共7页
Publications of the Yunnan Observatoty
