期刊
ASTROPHYSICAL JOURNAL
卷 670, 期 1, 页码 L17-L20出版社
UNIV CHICAGO PRESS
DOI: 10.1086/524137
关键词
binaries : close; stars : individual (GS 1826-24); stars : neutron; X-rays : binaries; X-rays : bursts
During a 200 ks observation with the XMM-Newton Reflection Grating Spectrometer, we detected 16 type I X-ray bursts from GS 1826-24. We combined the burst spectra in an attempt to measure the gravitational redshifts from the surface of the neutron star. We divided the composite GS 1826-24 burst spectrum into three groups based on the blackbody temperature during the bursts. The spectra do not show any obvious discrete absorption lines. We compare our observations with those of EXO 0748-676.
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