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Fallback Disk-Involved Spin-Down of Young Radio Pulsars
引用本文:Zi-Bo Jiang and Xiang-Dong Li Department of Astronomy,Nanjing University,Nanjing 210093,. Fallback Disk-Involved Spin-Down of Young Radio Pulsars[J]. 中国天文和天体物理学报, 2005, 5(5): 487-494
作者姓名:Zi-Bo Jiang and Xiang-Dong Li Department of Astronomy  Nanjing University  Nanjing 210093  
作者单位:Zi-Bo Jiang and Xiang-Dong Li Department of Astronomy,Nanjing University,Nanjing 210093;
基金项目:Supported by the National Natural Science Foundation of China.
摘    要:Disks originating from supernova fallback have been suggested to surround young neutron stars. Interaction between the disk and the magnetic field of the neutron star may considerably influence the evolution of the star through the so called propeller effect. There are many controversies about the efficiency of the propeller mechanism proposed in the literature. We investigate the fallback disk-involved spin-down of young pulsars. By comparing the simulated and measured results of pulsar evolution, we present some possible constraints on the propeller torques exerted by the disks on neutron stars.

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Fallback Disk-Involved Spin-Down of Young Radio Pulsars
Zi-Bo Jiang Xiang-Dong Li. Fallback Disk-Involved Spin-Down of Young Radio Pulsars[J]. Chinese Journal of Astronomy and Astrophysics, 2005, 5(5): 487-494
Authors:Zi-Bo Jiang Xiang-Dong Li
Affiliation:Department of Astronomy, Nanjing University, Nanjing 210093
Abstract:Disks originating from supernova fallback have been suggested to surround young neutron stars. Interaction between the disk and the magnetic field of the neutron star may considerably influence the evolution of the star through the so called propeller effect. There are many controversies about the efficiency of the propeller mechanism proposed in the literature. We investigate the fallback disk-involved spin-down of young pulsars. By comparing the simulated and measured results of pulsar evolution, we present some possible constraints on the propeller torques exerted by the disks on neutron stars.
Keywords:stars: magnetic fields - stars: neutron - pulsars: individual: PSRs B0532+21   B0833+45   B0540-69   B1509-58
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