Be‐X双星V635 CAS=4U0115+63瞬态前和瞬态期间的光学行为

A. Guarnieri, C. Bartolini, M. Teodorani, R. Silingardi, A. Piccioni
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摘要

本文介绍了1985-1990年在博洛尼亚天文台进行的Be - X双星系统V635 Cas光学成分观测的主要结果。三种变化特征较为突出:1)在数天的时间尺度上的光度变化;Ii)在大约一年的时间尺度上亮度的强烈增加;iii) Hα和Fe α等效宽度比值的幕式反演。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Optical behavior of the Be‐X binary V635 CAS=4U0115+63 before and during a transient phase
The main results of the observations of the optical component of the Be‐X binary system V635 Cas, carried out at the Bologna Observatory in the period 1985–1990 are presented. Three kinds of variable features were prominent: i) photometric variations on a time‐scale of several days; ii) a strong increase in luminosity on a time‐scale of about one year; iii) an episodic inversion of the ratio of the equivalent widths of Hα and Fe ii 6153.
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