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A New Kinematic Distance Estimator to the LMC

Andrew Gould
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Abstract

The distance to the Large Magellanic Cloud (LMC) can be directly determined by measuring three of its properties, its radial-velocity field, its mean proper motion, and the position angle ϕ_ph of its photometric line of nodes. Statistical errors of 2% are feasible based on proper motions obtained with any of several proposed astrometry satellites, the first possibility being the Full-Sky Astrometric Mapping Explorer (FAME). The largest source of systematic error is likely to be in the determination of ϕ_ph. I suggest two independent methods to measure ϕ_ph, one based on counts of clump giants and the other on photometry of clump giants. I briefly discuss a variety of methods to test for other sources of systematic errors.

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Andrew Gould. 1999-06-01. A New Kinematic Distance Estimator to the LMC. https://doi.org/10.1086/308169

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