Temporary Accretion Disk Around the X-ray Pulsar A0535+26

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Within the framework of our long multifrequency campaign of the X- Ray/Be System A0535+26/HDE245770, we present optical data showing the presence of a doubling in the HeI emission lines, which are usually absent. Such a doubling indicates the presence of a temporary accretion disk around the 104-s X-ray pulsar. We derive the possible dimensions of such a disk.

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