Can the Age Discrepancies of Neutron Stars Be Circumvented by an Accretion-assisted Torque? | Zendy

Yong Shi | Zendy; Renxin Xu | Zendy

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Can the Age Discrepancies of Neutron Stars Be Circumvented by an Accretion-assisted Torque?

Author(s) -

Yong Shi,

Renxin Xu

Publication year - 2003

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/379111

Subject(s) - neutron star , physics , astrophysics , torque , accretion (finance) , cyclotron , radius , magnetic dipole , stars , astronomy , dipole , nuclear physics , plasma , computer science , computer security , quantum mechanics , thermodynamics

It is found that 1E 1207.4-5209 could be a low-mass bare strange star if itssmall radius or low altitude cyclotron formation can be identified. The ageproblems of five sources could be solved by a fossil-disk-assisted torque. Themagnetic dipole radiation dominates the evolution of PSR B1757-24 at present,and the others are in propeller (or tracking) phases.

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