G. Vasisht et Ev. Gotthelf, THE DISCOVERY OF AN ANOMALOUS X-RAY PULSAR IN THE SUPERNOVA REMNANT KES-73, The Astrophysical journal, 486(2), 1997, pp. 129-132
We report the discovery of pulsed X-ray emission from the compact sour
ce 1E 1841-045, using data obtained with the Advanced Satellite for Co
smology and Astrophysics. The X-ray source is located in the center of
the small-diameter supernova remnant (SNR) Kes 73 and is very likely
to be the compact stellar remnant of the supernova that formed Kes 73.
The X-rays are pulsed with a period of similar or equal to 11.8 s and
a sinusoidal modulation of roughly 30%. We interpret this modulation
to be the rotation period of an embedded neutron star, and as such it
would be the longest spin period for an isolated neutron star to date.
This is especially remarkable since the surrounding SNR is very young
, similar to 2000 yr old. We suggest that the observed characteristics
of this object are best understood within the framework of a neutron
star with an enormous dipolar magnetic field, B similar or equal to 8
x 10(14) G.