期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 353, 期 4, 页码 1286-1292出版社
BLACKWELL PUBLISHING LTD
DOI: 10.1111/j.1365-2966.2004.08150.x
关键词
stars : emission-line, Be; Magellanic Clouds; X-rays : binaries
Three new X-ray pulsars have been detected in the Small Magellanic Cloud (SMC) and the positions of two others have been determined, with archive Chandra data. A series of five observations of the SMC took place between 2002 May and October. Analysis of these data has revealed three previously unknown X-ray pulsars at pulse periods of 34, 503 and 138 s. The position of pulsar XTE J0052-725, which was originally detected by RXTE on 2002 June 19, was also accurately determined and a previously detected 7.78-s RXTE pulsar was identified as the source SMC X-3.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据