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
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