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PDF-).Thisisconsistentwiththestandardmodelfortheirorigininwhichan PDF document

RL28104kmjust40ofthatofJupiterOntheotherhandforapulsarmassmp2 canbederivedbycombiningtheaboveequations304623GP2b23gcm34Thisdensityisindependentoftheinclinationangleandthepulsarmassa

RL=2.8$104km just40%ofthatofJupiter.Ontheotherhand forapulsarmassmp=2 ))canbederivedbycombiningtheaboveequations.#=3"0.4623GP2b=23gcm!3(4)Thisdensityisindependentoftheinclinationangleandthepulsarmassa

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