X 1822-371的星历更新

The evolution of X‐ray binaries Pub Date : 2008-05-12 DOI:10.1063/1.46038

C. Hellier, A. Smale

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引用次数: 2

摘要

X 1822-371轨道周期的增加(时间尺度为3×106年)被ROSAT的新观测证实。与其他一些lmxb相比，简单的二次星历表仍然很适合日食时间。

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An ephemeris update for X 1822–371

The increase in the orbital period of X 1822–371 with a timescale of 3×106 yrs is confirmed by a new ROSAT observation. In contrast to some other LMXBs, a simple quadratic ephemeris remains a good fit to the eclipse timings.

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The evolution of X‐ray binaries

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