With their huge number of stars,many of which are members of binary systems,globular clusters provide a rich source of pulsar progenitors.Those in binary systems will evolve,often spinning up or“recycling”the pulsar...With their huge number of stars,many of which are members of binary systems,globular clusters provide a rich source of pulsar progenitors.Those in binary systems will evolve,often spinning up or“recycling”the pulsar through accretion of mass and angular momentum from the evolving companion star.If this accretion process goes through completion.展开更多
The intensity distribution of emission beam and the new radio luminosity formula of pulsars are presented on the basis of the geometrical relations of polar-cap model. There are 102 pulsars with the new radio luminosi...The intensity distribution of emission beam and the new radio luminosity formula of pulsars are presented on the basis of the geometrical relations of polar-cap model. There are 102 pulsars with the new radio luminosity values. It is shown that the radio luminosity can be described only by one relation L∞(B/p^2)^(1.1) or L∞Q'^(-1.4) over the whole range of period and period derivatives, which is contrary to other recently suggested luminosity laws.展开更多
基金supported by the Australian National Data Service(ANDS).ANDS is supported by the Australian Government through the National Collaborative Research Infrastructure Strategy Program and the Education Investment Fund(EIF)Super Science Initiative 19the UK's AstroGrid Virtual Observatory Project,which is funded by the Science and Technology Facilities Council andthrough the EU's Framework 6 programme+1 种基金part of the Australia Telescope,whichis funded by the Commonwealth of Australia for operation as a National Facility managed by the Commonwealth Scientific and Industrial Research Organisation(CSIRO)GH is the recipient of an Australian Research CouncilQEII Fellowship(#DP0878388)
文摘With their huge number of stars,many of which are members of binary systems,globular clusters provide a rich source of pulsar progenitors.Those in binary systems will evolve,often spinning up or“recycling”the pulsar through accretion of mass and angular momentum from the evolving companion star.If this accretion process goes through completion.
基金Project supported by the National Natural Science Foundation of China.
文摘The intensity distribution of emission beam and the new radio luminosity formula of pulsars are presented on the basis of the geometrical relations of polar-cap model. There are 102 pulsars with the new radio luminosity values. It is shown that the radio luminosity can be described only by one relation L∞(B/p^2)^(1.1) or L∞Q'^(-1.4) over the whole range of period and period derivatives, which is contrary to other recently suggested luminosity laws.
