Recent observations of EXO 2030+375 with BATSE

The evolution of X‐ray binaries Pub Date : 2008-05-12 DOI:10.1063/1.46018

M. Stollberg, W. Paciesas, M. Finger, G. Fishman, R. Wilson, B. A. Harmon, C. Wilson

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Abstract

The transient x‐ray pulsar EXO 2030+375 has been detected in the Large Area Detectors (LADs) of BATSE during twelve outbursts from February 1992 to July 1993. These data have been fit to a model of the pulsar’s rotational phase which assumes an independent torque for each outburst. An intensity history, a pulse period history, a pulsed fraction, and the latest orbit parameters resulting from this fit are presented.

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用BATSE对EXO 2030+375的最新观测

从1992年2月到1993年7月，BATSE的大面积探测器(LADs)在12次爆发中发现了瞬态x射线脉冲星EXO 2030+375。这些数据已经适合于脉冲星的旋转相位模型，该模型假设每次爆发都有独立的扭矩。给出了强度历史、脉冲周期历史、脉冲分数和由该拟合得到的最新轨道参数。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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The evolution of X‐ray binaries

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