Optical identifications of M31 sources

E. Magnier
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引用次数: 1

Abstract

The Einstein X‐ray Observatory Satellite provided the first detection of isolated x‐ray sources in the Andromeda Galaxy. Recent ROSAT observations have provided observations of the x‐ray binaries in M31 complete to Lx∼1034 erg sec−1, and are sensitive enough to detect many supernova remnants and other x‐ray sources. Optical identifications are crucial to identify or confirm the identifications of these sources. This article reviews the search for optical counterparts to the Einstein x‐ray sources and discusses the ongoing efforts of the MIT‐UvA‐MPE group to identify optical counterparts to the ROSAT x‐ray sources.
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M31光源的光学识别
爱因斯坦X射线观测卫星首次探测到仙女座星系中孤立的X射线源。最近的ROSAT观测提供了M31中x射线双星的观测结果,完整到Lx ~ 1034 erg sec−1,并且足够灵敏,可以探测到许多超新星遗迹和其他x射线源。光学识别对于识别或确认这些源的识别至关重要。本文回顾了寻找爱因斯坦x射线源的光学对偶体的研究,并讨论了MIT - UvA - MPE小组为识别ROSAT x射线源的光学对偶体所做的努力。
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