Microlensing and Galactic Structure

Because we know little about the Galactic force-field away from the plane, the Galactic mass distribution is very ill-determined. I show that a microlensing survey of galaxies closer than 50 Mpc would enable us to map in three dimensions the Galactic density of stellar mass, which should be strictly...

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Bibliographic Details
Main Author: Binney, J
Format: Journal article
Published: 2000
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author Binney, J
author_facet Binney, J
author_sort Binney, J
collection OXFORD
description Because we know little about the Galactic force-field away from the plane, the Galactic mass distribution is very ill-determined. I show that a microlensing survey of galaxies closer than 50 Mpc would enable us to map in three dimensions the Galactic density of stellar mass, which should be strictly less than the total mass density. A lower limit can be placed on the stellar mass needed at R
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spelling oxford-uuid:69bab480-6165-43be-88d1-65e28caea2992022-03-26T18:52:50ZMicrolensing and Galactic StructureJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:69bab480-6165-43be-88d1-65e28caea299Symplectic Elements at Oxford2000Binney, JBecause we know little about the Galactic force-field away from the plane, the Galactic mass distribution is very ill-determined. I show that a microlensing survey of galaxies closer than 50 Mpc would enable us to map in three dimensions the Galactic density of stellar mass, which should be strictly less than the total mass density. A lower limit can be placed on the stellar mass needed at R
spellingShingle Binney, J
Microlensing and Galactic Structure
title Microlensing and Galactic Structure
title_full Microlensing and Galactic Structure
title_fullStr Microlensing and Galactic Structure
title_full_unstemmed Microlensing and Galactic Structure
title_short Microlensing and Galactic Structure
title_sort microlensing and galactic structure
work_keys_str_mv AT binneyj microlensingandgalacticstructure