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The Effect of Differential Limb Magnification On Abundance Analysis of Microlensed Dwarf Stars

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dc.creator Johnson, Jennifer A.
dc.creator Dong, Subo
dc.creator Gould, Andrew
dc.date.accessioned 2011-02-07T17:51:00Z
dc.date.available 2011-02-07T17:51:00Z
dc.date.issued 2010-04-20
dc.identifier.citation Jennifer A. Johnson, Subo Dong, and Andrew Gould, "The Effect of Differential Limb Magnification On Abundance Analysis of Microlensed Dwarf Stars," The Astrophysical Journal 713, no. 2 (2010), doi:10.1088/0004-637X/713/2/713 en_US
dc.identifier.issn 1538-4357
dc.identifier.uri http://hdl.handle.net/1811/47808
dc.description.abstract Finite source effects can be important in observations of gravitational microlensing of stars. Near caustic crossings, for example, some parts of the source star will be more highly magnified than other parts. The spectrum of the star is then no longer the same as when it is unmagnified, and measurements of the atmospheric parameters and abundances will be affected. The accuracy of abundances measured from spectra taken during microlensing events has become important recently because of the use of highly magnified dwarf stars to probe abundance ratios and the abundance distribution in the Galactic bulge. In this paper, we investigate the importance of finite source effects on spectra by using magnification profiles motivated by two events to synthesize spectra for dwarfs between 5000 K and 6200 K at solar metallicity. We adopt the usual techniques for analyzing the microlensed dwarfs, namely, spectroscopic determination of temperature, gravity, and microturbulent velocity, relying on equivalent widths. We find that ignoring the finite source effects for the more extreme case results in errors in T_eff <45 K, in log g of <0.1 dex, and in ξ of <0.1 km s^–1. In total, changes in equivalent widths lead to small changes in atmospheric parameters and changes in abundances of <0.06 dex, with changes in [Fe I/H] of <0.03 dex. For the case with a larger source-lens separation, the error in [Fe I/H] is <0.01 dex. This latter case represents the maximum effect seen in events whose light curves are consistent with a point-source lens, which includes the majority of microlensed bulge dwarfs published so far. en_US
dc.language.iso en_US en_US
dc.publisher American Astronomical Society en_US
dc.subject Galaxy: bulge en_US
dc.subject gravitational lensing: micro en_US
dc.subject line: profiles en_US
dc.subject stars: abundances en_US
dc.subject stars: atmospheres en_US
dc.title The Effect of Differential Limb Magnification On Abundance Analysis of Microlensed Dwarf Stars en_US
dc.type Article en_US
dc.identifier.doi 10.1088/0004-637X/713/2/713
dc.identifier.osuauthor johnson.3064
dc.identifier.osuauthor dong.59
dc.identifier.osuauthor gould.34