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- Anomalous_X-ray_pulsar abstract "Anomalous X-ray Pulsars (AXPs) are now widely believed to be magnetars—young, isolated, highly magnetized neutron stars. These energetic X-ray pulsars are characterized by slow rotation periods of ~2–12 seconds and large magnetic fields of ~1013–1015 gauss (1 to 100 gigateslas). There are currently (as of 2009) 9 known and 1 candidate AXPs. The identification of AXPs with magnetars was motivated by their similarity to another enigmatic class of sources, the soft gamma repeaters.".
- Anomalous_X-ray_pulsar wikiPageExternalLink ucsd.pdf.
- Anomalous_X-ray_pulsar wikiPageExternalLink research.php?subdir=strangeQuarkStars.
- Anomalous_X-ray_pulsar wikiPageExternalLink magnetar.pdf.
- Anomalous_X-ray_pulsar wikiPageID "1250374".
- Anomalous_X-ray_pulsar wikiPageRevisionID "593204318".
- Anomalous_X-ray_pulsar hasPhotoCollection Anomalous_X-ray_pulsar.
- Anomalous_X-ray_pulsar subject Category:Anomalous_X-ray_pulsars.
- Anomalous_X-ray_pulsar subject Category:Magnetars.
- Anomalous_X-ray_pulsar subject Category:Pulsars.
- Anomalous_X-ray_pulsar subject Category:Star_types.
- Anomalous_X-ray_pulsar subject Category:X-ray_pulsars.
- Anomalous_X-ray_pulsar type AnomalousX-rayPulsars.
- Anomalous_X-ray_pulsar type CelestialBody109239740.
- Anomalous_X-ray_pulsar type NaturalObject100019128.
- Anomalous_X-ray_pulsar type NeutronStar109369692.
- Anomalous_X-ray_pulsar type Object100002684.
- Anomalous_X-ray_pulsar type PhysicalEntity100001930.
- Anomalous_X-ray_pulsar type Pulsar109400987.
- Anomalous_X-ray_pulsar type Pulsars.
- Anomalous_X-ray_pulsar type Star109444100.
- Anomalous_X-ray_pulsar type Whole100003553.
- Anomalous_X-ray_pulsar type X-rayPulsars.
- Anomalous_X-ray_pulsar comment "Anomalous X-ray Pulsars (AXPs) are now widely believed to be magnetars—young, isolated, highly magnetized neutron stars. These energetic X-ray pulsars are characterized by slow rotation periods of ~2–12 seconds and large magnetic fields of ~1013–1015 gauss (1 to 100 gigateslas). There are currently (as of 2009) 9 known and 1 candidate AXPs. The identification of AXPs with magnetars was motivated by their similarity to another enigmatic class of sources, the soft gamma repeaters.".
- Anomalous_X-ray_pulsar label "Anomalny pulsar rentgenowski".
- Anomalous_X-ray_pulsar label "Anomalous X-ray pulsar".
- Anomalous_X-ray_pulsar label "Pulsar X anormal".
- Anomalous_X-ray_pulsar label "Аномальный рентгеновский пульсар".
- Anomalous_X-ray_pulsar label "特異X線パルサー".
- Anomalous_X-ray_pulsar sameAs Anomalous_X-Ray_Pulsar.
- Anomalous_X-ray_pulsar sameAs Pulsar_X_anormal.
- Anomalous_X-ray_pulsar sameAs 特異X線パルサー.
- Anomalous_X-ray_pulsar sameAs Anomalny_pulsar_rentgenowski.
- Anomalous_X-ray_pulsar sameAs m.04m488.
- Anomalous_X-ray_pulsar sameAs Q2985002.
- Anomalous_X-ray_pulsar sameAs Q2985002.
- Anomalous_X-ray_pulsar sameAs Anomalous_X-ray_pulsar.
- Anomalous_X-ray_pulsar wasDerivedFrom Anomalous_X-ray_pulsar?oldid=593204318.
- Anomalous_X-ray_pulsar isPrimaryTopicOf Anomalous_X-ray_pulsar.