银河系星际尘埃中可能的双星V335 Vul的观测
天体物理学
2007-05-23 v1
摘要
我们呈现了一组关于疑似双星V335 Vul的可见光和CCD VRI观测。长期光度测量表明，这可能是典型的Mira或SRa脉冲星。高速V波段CCD光度测量没有发现超过0.02 mag的异常现象。
引用
@article{arxiv.astro-ph/0210585,
title = {Observations of possible symbiotic star V335 Vul},
author = {Petr Sobotka and Ondrej Pejcha and Ladislav Smelcer and Pavel Marek},
journal= {arXiv preprint arXiv:astro-ph/0210585},
year = {2007}
}
备注
4 pages, 2 Postscript figures, to appear in the proceedings of "Symbiotic stars probing stellar evolution", R.L.M.Corradi, J.Mikolajewska, T.J.Mahoney eds., 2002, ASP Conference Series, in press