Modelling the Galactic bar using OGLE-II Red Clump Giant Stars
Abstract
Red clump giant stars can be used as distance indicators to trace the mass distribution of the Galactic bar. We use RCG stars from 44 bulge fields from the OGLE-II microlensing collaboration database to constrain analytic tri-axial models for the Galactic bar. We find the bar major axis is oriented at an angle of 24 - 27 degrees to the Sun-Galactic centre line-of-sight. The ratio of semi-major and semi-minor bar axis scale lengths in the Galactic plane x_0, y_0, and vertical bar scale length z_0, is x_0 : y_0 : z_0 = 10 : 3.5 : 2.6, suggesting a slightly more prolate bar structure than the working model of Gerhard (2002) which gives the scale length ratios as x_0 : y_0 : z_0 = 10 : 4 : 3 .
Cite
@article{arxiv.0704.1614,
title = {Modelling the Galactic bar using OGLE-II Red Clump Giant Stars},
author = {Nicholas J. Rattenbury and Shude Mao and Takahiro Sumi and Martin C. Smith},
journal= {arXiv preprint arXiv:0704.1614},
year = {2009}
}
Comments
15 pages, 10 figures, accepted for publication in MNRAS. Supplementary material available online: 10 pages, 10 figures