Title of article
A Supernova Remnant Collision with a Stellar Wind
Author/Authors
Vel?zquez، Pablo F. نويسنده , , Koenigsberger، Gloria نويسنده , , Raga، Alejandro C. نويسنده ,
Issue Information
روزنامه با شماره پیاپی 1 سال 2003
Pages
-283
From page
284
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
X-rays: ISM , Supernova remnants , stars: winds, outflows , stars: individual (HD 5980) , Magellanic Clouds
Journal title
Astrophysical Journal
Serial Year
2003
Journal title
Astrophysical Journal
Record number
73757
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