• Title of article

    Understanding the Radio Emission Geometry of Multiple-Component Radio Pulsars from Retardation and Aberration Effects

  • Author/Authors

    Gupta، Y. نويسنده , , Gangadhara، R. T. نويسنده ,

  • Issue Information
    روزنامه با شماره پیاپی 1 سال 2003
  • Pages
    -417
  • From page
    418
  • To page
    0
  • Abstract
    Microlensing surveys derive the microlensing optical depth toward various directions such as the Galactic center from the distribution of observed Einstein radius crossing times. I show that the formula that is being used is invalid for "exotic" lensing events. The corrected formula is derived. The "parallax" effect (Earth motion) requires no correction. Corrections for the finite sizes of sources and wide binary lenses are small (typically less than 1%), except for blended events. Corrections for intermediate-type binaries such as MACHO LMC-9 can be substantial.
  • Keywords
    stars: neutron , radiation mechanisms: nonthermal , stars: magnetic fields , pulsars: general
  • Journal title
    Astrophysical Journal
  • Serial Year
    2003
  • Journal title
    Astrophysical Journal
  • Record number

    73803