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Rotation-powered pulsar (RPP or "radio pulsar"): [71] neutron stars that emit directed pulses of radiation towards us at regular intervals (due to their strong magnetic fields) Rotating radio transient (RRATs): [71] thought to be pulsars which emit more sporadically and/or with higher pulse-to-pulse variability than the bulk of the known pulsars Magnetar: a neutron star with an extremely strong magnetic field (1,000 times more than a regular neutron star), and long rotation periods (5 to 12 seconds) Soft gamma repeater (SGR) [67] Anomalous X-ray pulsar (AXP) [67] Radio-quiet neutron stars X-ray-dim isolated neutron stars [71] Central compact objects in supernova remnants (CCOs in SNRs): young, radio-quiet non-pulsating X-ray sources, thought to be isolated neutron stars surrounded by supernova remnants [71] X-ray pulsars or "accretion-powered pulsars": a class of X-ray binaries Low-mass X-ray binary pulsars: a class of low-mass X-ray binaries (LMXB), a pulsar with a main-sequence star, white dwarf or red giant Millisecond pulsar (MSP) ("recycled pulsar") X-ray burster: a neutron star with a low-mass binary companion from which matter is accreted resulting in irregular bursts of energy from the surface of the neutron star Intermediate-mass X-ray binary pulsars: a class of intermediate-mass X-ray binaries (IMXB), a pulsar with an intermediate mass star High-mass X-ray binary pulsars: a class of high-mass X-ray binaries (HMXB), a pulsar with a massive star Binary pulsars: a pulsar with a binary companion, often a white dwarf or neutron star

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Farrelly MC, Davis KC, Haviland ML, Messeri P, Healton CG

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