A Pattern Speed in the Galaxy's OH/IR Stars
arXiv:astro-ph/0203380 · doi:10.1007/10899892_3
Abstract
We use the Tremaine-Weinberg method, adapted to the Milky Way, to measure a pattern speed in OH/IR stars located in the inner MW.
2 pages, 1 figure. Contribution to `The Mass of Galaxies at Low and High Redshift', ed. R. Bender & A. Renzini, ESO Astrophysics Symposia (Springer-Verlag), to appear