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- CXOU_J164710.2-455216 abstract "CXOU J164710.2-455216 is an anomalous X-ray pulsar in the massive galactic open cluster Westerlund 1. It is the brightest X-ray source in the cluster, and was discoveredin 2005 in observations made by the Chandra X-ray observatory. The Westerlund 1 cluster is believed to have formed in a single burst of star formation, implying that the progenitor star must have had a mass in excess of 40 solar masses. The fact that a neutron star was formed instead of a black hole implies that more than 95% of the star's original mass must have been lost before or during the supernova that produced the magnetar.On 21 September 2006 the Swift satellite detected a 20ms soft Gamma-ray burst in Westerlund 1. Fortuitously, XMM-Newton observations had been made four days earlier, and repeat observations 1.5 days after the burst revealed the magnetar to be the source of the burst, with the X-ray luminosity increasing by a factor of 100 during the outburst.".
- CXOU_J164710.2-455216 wikiPageExternalLink cxo-j164710.2-455216.shtml.
- CXOU_J164710.2-455216 wikiPageID "16079402".
- CXOU_J164710.2-455216 wikiPageRevisionID "601857726".
- CXOU_J164710.2-455216 appmag ">18.5".
- CXOU_J164710.2-455216 constell Ara_(constellation).
- CXOU_J164710.2-455216 distLy "approx. 16000".
- CXOU_J164710.2-455216 distPc "approx. 5000".
- CXOU_J164710.2-455216 epoch "J2000.0".
- CXOU_J164710.2-455216 rotation "10.6105".
- CXOU_J164710.2-455216 type Neutron_star.
- CXOU_J164710.2-455216 subject Category:Ara_(constellation).
- CXOU_J164710.2-455216 subject Category:Magnetars.
- CXOU_J164710.2-455216 subject Category:Neutron_stars.
- CXOU_J164710.2-455216 subject Category:Pulsars.
- CXOU_J164710.2-455216 subject Category:Variable_stars.
- CXOU_J164710.2-455216 type CelestialBody.
- CXOU_J164710.2-455216 type Star.
- CXOU_J164710.2-455216 type PhysicalBody.
- CXOU_J164710.2-455216 comment "CXOU J164710.2-455216 is an anomalous X-ray pulsar in the massive galactic open cluster Westerlund 1. It is the brightest X-ray source in the cluster, and was discoveredin 2005 in observations made by the Chandra X-ray observatory. The Westerlund 1 cluster is believed to have formed in a single burst of star formation, implying that the progenitor star must have had a mass in excess of 40 solar masses.".
- CXOU_J164710.2-455216 label "CXO J164710.2-455216".
- CXOU_J164710.2-455216 label "CXO J164710.2-455216".
- CXOU_J164710.2-455216 label "CXOU J164710.2-455216".
- CXOU_J164710.2-455216 sameAs CXO_J164710.2-455216.
- CXOU_J164710.2-455216 sameAs CXO_J164710.2-455216.
- CXOU_J164710.2-455216 sameAs m.03qnhw8.
- CXOU_J164710.2-455216 sameAs Q5096753.
- CXOU_J164710.2-455216 sameAs Q5096753.
- CXOU_J164710.2-455216 wasDerivedFrom CXOU_J164710.2-455216?oldid=601857726.
- CXOU_J164710.2-455216 isPrimaryTopicOf CXOU_J164710.2-455216.
- CXOU_J164710.2-455216 name "CXOU J164710.2-455216".