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About: PSR J0348+0432     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatPulsars, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatMillisecondPulsarsyago:WikicatNeutronStarsyago:CelestialBody109239740yago:NaturalObject100019128yago:NeutronStar109369692yago:Object100002684yago:PhysicalEntity100001930yago:Pulsar109400987staryago:Star109444100yago:Whole100003553yago:WikicatPulsars New Facet based on Instances of this Class

PSR J0348+0432 is a pulsar–white dwarf binary system in the constellation Taurus. It was discovered in 2007 with the National Radio Astronomy Observatory's Robert C. Byrd Green Bank Telescope in a drift-scan survey. The notable feature of this binary pulsar is its combination of high neutron-star mass and short orbital period: 2 hours and 27 minutes.This allowed a measurement of the orbital decay due to the emission of gravitational waves, as observed for PSR B1913+16 and PSR J0737−3039.