A New Kinematic Distance Estimator to the LMC
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 \phi_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 \phi_ph. I suggest two independent methods to measure \phi_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.
Cite
@article{arxiv.astro-ph/9906021,
title = {A New Kinematic Distance Estimator to the LMC},
author = {Andrew Gould},
journal= {arXiv preprint arXiv:astro-ph/9906021},
year = {2009}
}
Comments
submitted to ApJ, 13 pages