A SPECTROGRAPHIC ANALYSIS OF NOVA VULPECULAE 1968, NO. 1
A SPECTROGRAPHIC ANALYSIS OF NOVA VULPECULAE 1968, NO. 1
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新星狐的光谱分析 1968，NO。
DOI：
10.1086/128937
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发表时间：
1970
影响因子：
3.5
通讯作者：
J. Hutchings
中科院分区：
文献类型：
--
作者：
J. Hutchings
J. B. 1“'UTHANGS自治领天体物理观测站Beceice /joi tory 5，1970总结了新星径向速度测量、谱线识别和中等色散谱线轮廓还原的结果。速度关系和线的轮廓一起讨论公布的新星的光变曲线。推导出两个主要的壳层被抛出并加速离开，并导出了在outhurst后的前100天的几何和物理参数，讨论了加速的过程，并与1967年的缓慢的Nova Delphini进行了对比。
J. B. 1"'UTCHINGS Dominion Astrophysical Observatory Beceice /joi tory 5, 1970 The results of radial velocity measurements, line identifications, and line profile reductions on medium dispersion spectra of the nova are summarized. The velocity relations and line profiles are discussed together with published light curves of the nova. It is deduced that two main shells were ejected and accelerated away from , and geometric and physical parameters are derived for the first 100 days after outhurst The of the acceleration is discussed and contrasted with the slow Nova Delphini 1967.