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Detection of 33.8 ms X-ray pulsations in SAX J0635+0533

We revisited the BeppoSAX observation of SAX J0635+0533, suggested as a possible counterpart to the gamma-ray source 2EG J0635+0521. We have discovered a 33.8 ms pulsation from the source and derived an improved position, consistent with the location of the Be star proposed as a binary companion. We interpret the periodicity as the spin period of a neutron star in a binary system with a Be companion.

preprint1999arXivOpen access
G. CusumanoM. C. MaccaroneL. NicastroB. SaccoP. Kaaret
astro-ph
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Open access5 authors1 topic
Imported metadata coverageMissing code, dataset, citation and institution fields are tracked without dominating the paper.Details
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G. CusumanoM. C. MaccaroneL. NicastroB. SaccoP. Kaaret

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