Long-Term Photometry of Very Slow Novae
Long-Term Photometry of Very Slow Novae
复制标题
非常慢的新星的长期光度测量
DOI：
10.1515/astro-2017-0089
复制
发表时间：
2003
期刊：
影响因子：
0.7
通讯作者：
M. Vaňko
中科院分区：
文献类型：
--
作者：
D. Chochol;T. Pribulla;S. Parimucha;M. Vaňko
利用经典新星V723 Cas和共生新星V1329 Cyg、PU Vul、V1016 Cyg和HM Sge的长期照相、光电和近期CCD测光资料，计算了它们的轨道周期。在这些系统中的第三个组件的存在赞成的论据。物理过程，负责的亮度变化，进行了讨论。
Abstract Long-term photographic, photoelectric and recent CCD photometry of the classical nova V723 Cas and symbiotic novae V1329 Cyg, PU Vul, V1016 Cyg and HM Sge were used to find their orbital periods. The arguments in favor of the presence of the third components in these systems are given. Physical processes, responsible for the brightness variations, are discussed.