1997/07/16 by Seunghun Lee, Cheongho Han, Lee, Seunghun +1
Physics and Astronomy · #Adaptive optics and wavefront sensing #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Stellar, planetary, and galactic studies #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9707178
14 pages, 2 figures, and 3 Tables, submitted to APJ on Jul 16th 1997
arxiv created 1997/07/16 · openalex publication_date 1997/07/16 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
The most important uncertainty in the results of gravitational microlensing experiments comes from the difficulties of photometry caused by blending of source stars. Recently Nemiroff (1997) pointed out that the results of microlensing experiments can also be affected by the blending of light from the lens itself if a significant fraction of lenses are composed of stars. In this paper, we estimate the effects of lens blending on the optical depth determination and the derived matter distribution toward the Galactic bulge by using realistic models of the lens matter distribution and a well-constrained stellar luminosity function. We find that the effect of lens blending is largest for lenses located in the Galactic disk. However, lens blending does not seriously affect both the determination of the optical depth and the Galactic matter distribution. The decrease in optical depth is ∼ 10% even under the extreme assumption that lenses are totally composed of stars and disk matter distribution follows a maximal disk model, in which the lens blending effect is most severe.