Of Galactic Novae
Of Galactic Novae
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银河新星
DOI：
10.1007/978-94-009-3753-6_16
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发表时间：
1987
期刊：
影响因子：
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通讯作者：
M. Snijders
中科院分区：
文献类型：
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作者：
S. Starrfield;M. Snijders
经典新星爆发是星系中发生的第二剧烈的爆炸，其剧烈程度仅次于超新星爆炸。然而，新星相对较近，新星爆发比超新星爆发更频繁，因此 Payne-Gaposchkin (1957) 和 McLaughlin (1960) 列出并讨论了 200 多个爆发。第一个新星紫外线（以下简称：UV）研究是 1970 年 FH Ser 爆发的研究（Gallagher 和 Code，1974 年），这是由 OAO-A2 卫星完成的宽带光度测量。第一个紫外光谱研究是哥白尼 1975 年对 V1500 Cyg 进行的研究（Jenkins 等人，1977 年），但它是一颗速度如此之快的新星，以至于拍摄光谱时唯一可见的线是 Mg II λ2800。 Nova Cyg 也通过 ANS 卫星进行了研究（Wu 和 Kester，1975）。
The classical nova outburst is the second most violent explosion that occurs in a galaxy and its violence is exceeded only by a supernova explosion. However, novae are relatively nearby and a nova outburst occurs much more frequently than a supernova outburst so that there are more than 200 outbursts tabulated and discussed by Payne-Gaposchkin (1957) and McLaughlin (1960). The first ultraviolet (hereafter: UV) study of a nova was that of the 1970 outburst of FH Ser (Gallagher and Code, 1974) and that was broad band photometry done by the OAO—A2 satellite. The first UV spectroscopic study was that of V1500 Cyg 1975 done with Copernicus (Jenkins et al., 1977) but it was such a fast nova that the only line visible when the spectrum was taken was Mg II λ2800. Nova Cyg was also studied with the ANS satellite (Wu and Kester, 1975).