Title of article :
A Compact Central Object in the Supernova Remnant Kesteven 79
Author/Authors :
Sun، M. نويسنده , , Slane، P. O. نويسنده , , Seward، F. D. نويسنده , , Smith، R. K. نويسنده ,
Issue Information :
روزنامه با شماره پیاپی 1 سال 2003
Pages :
-413
From page :
414
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 :
Supernova remnants , ISM: individual (Kesteven 79) , stars: neutron , X-rays: stars
Journal title :
Astrophysical Journal
Serial Year :
2003
Journal title :
Astrophysical Journal
Record number :
73800
Link To Document :
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