A 0535+26: a historical tour

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

We present a long-term timing analysis of the accreting X-ray pulsar A 0535+26 using data from Fermi/GBM, RXTE and Swift/BAT. A new orbital ephemeris is obtained from normal outbursts experienced by this source since 2005, and a long-term pulse profile study is carried out. In this study we include results from the current outburst. This outburst is believed to be much larger than the previous ones.

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