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Detection of 33.8 Millisecond X-Ray Pulsations in SAX J0635+0533
Author(s) -
G. Cusumano,
M. C. Maccarone,
L. Nicastro,
B. Sacco,
P. Kaaret
Publication year - 2000
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/312413
Subject(s) - neutron star , millisecond , physics , astrophysics , binary number , x ray binary , astronomy , position (finance) , x ray , nuclear physics , mathematics , finance , economics , arithmetic
We revisited the BeppoSAX observation of SAX J0635+0533, which was 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.

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