Enigmatic sub-luminous accreting neutron stars in our Galaxy

Details Enigmatic sub-luminous accreting neutron stars in our Galaxy Enigmatic sub-luminous accreting neutron stars in our Galaxy

2008-01-07

arxiv.org/abs/0801.0953v1

AIP Conf.Proc.1010:382-386,2008

Astronomy and Astrophysics

Astrophysics

Conference proceedings from 'A Population Explosion: The Nature and Evolution of X-ray Binaries in Diverse Environments', 28 O

Scientific paper

10.1063/1.2945081

During the last few years a class of enigmatic sub-luminous accreting neutron
stars has been found in our Galaxy. They have peak X-ray luminosities (2-10
keV) of a few times 1E34 erg/s to a few times 1E35 erg/s, and both persistent
and transient sources have been found. I present a short overview of our
knowledge of these systems and what we can learn from them.

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