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- SWIFT_J1756.9-2508 abstract "SWIFT J1756.9-2508 is a millisecond pulsar with a rotation frequency of 182 Hz (period of 5.5 ms). It was discovered in 2007 by the Swift Gamma-Ray Burst Explorer and found to have a companion with a mass between 0.0067 and 0.030 solar masses. It is thought that the companion is the remnant of a former companion star, now stripped down to a planetary-mass core. The pulsar is accreting mass from this companion, resulting in occasional violent outbursts from the accumulated material on the neutron star.".
- SWIFT_J1756.9-2508 wikiPageExternalLink lab_bib.
- SWIFT_J1756.9-2508 wikiPageExternalLink pulsar-has-almost-completely-devoured-a-star.
- SWIFT_J1756.9-2508 wikiPageID "13237359".
- SWIFT_J1756.9-2508 wikiPageRevisionID "599734776".
- SWIFT_J1756.9-2508 constell Sagittarius_(constellation).
- SWIFT_J1756.9-2508 epoch Epoch_(astronomy).
- SWIFT_J1756.9-2508 hasPhotoCollection SWIFT_J1756.9-2508.
- SWIFT_J1756.9-2508 subject Category:Accreting_millisecond_pulsars.
- SWIFT_J1756.9-2508 subject Category:Sagittarius_(constellation).
- SWIFT_J1756.9-2508 subject Category:X-ray_binaries.
- SWIFT_J1756.9-2508 type CelestialBody.
- SWIFT_J1756.9-2508 type Star.
- SWIFT_J1756.9-2508 type PhysicalBody.
- SWIFT_J1756.9-2508 comment "SWIFT J1756.9-2508 is a millisecond pulsar with a rotation frequency of 182 Hz (period of 5.5 ms). It was discovered in 2007 by the Swift Gamma-Ray Burst Explorer and found to have a companion with a mass between 0.0067 and 0.030 solar masses. It is thought that the companion is the remnant of a former companion star, now stripped down to a planetary-mass core.".
- SWIFT_J1756.9-2508 label "SWIFT J1756.9-2508".
- SWIFT_J1756.9-2508 sameAs m.03bzv7k.
- SWIFT_J1756.9-2508 sameAs Q7395189.
- SWIFT_J1756.9-2508 sameAs Q7395189.
- SWIFT_J1756.9-2508 wasDerivedFrom SWIFT_J1756.9-2508?oldid=599734776.
- SWIFT_J1756.9-2508 isPrimaryTopicOf SWIFT_J1756.9-2508.
- SWIFT_J1756.9-2508 name "SWIFT J1756.9-2508".