(Anomalous) X-ray Pulsars

Details (Anomalous) X-ray Pulsars (Anomalous) X-ray Pulsars

2004-02-08

arxiv.org/abs/astro-ph/0402176v1

Astronomy and Astrophysics

Astrophysics

10 pages, 5 figures. To appear in Proc. of the BeppoSAX Symposium: "The Restless High-Energy Universe," Eds. E.P.J. van den He

Scientific paper

10.1016/j.nuclphysbps.2004.04.08

We review the observational properties of the class of young neutron stars
known as "anomalous X-ray pulsars," emphasizing the tremendous progress that
has been made in recent years, and explain why these objects, like the "soft
gamma repeaters," are today thought to be young, isolated, ultrahigh magnetic
field neutron stars, or "magnetars."

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