Investigation of the Galactic Bar based on Photometry and Stellar Proper Motions
arXiv:1402.3153 · doi:10.1134/S1063773714030037
Abstract
A new method for selecting stars in the Galactic bar based on 2MASS infrared photometry in combination with stellar proper motions from the Kharkiv XPM catalogue has been implemented. In accordance with this method, red clump and red giant branch stars are preselected on the color -- magnitude diagram and their photometric distances are calculated. Since the stellar proper motions are indicators of a larger velocity dispersion toward the bar and the spiral arms compared to the stars with circular orbits, applying the constraints on the proper motions of the preselected stars that take into account the Galactic rotation has allowed the background stars to be eliminated. Based on a joint analysis of the velocities of the selected stars and their distribution on the Galactic plane, we have confidently identified the segment of the Galactic bar nearest to the Sun with an orientation of 20--25 with respect to the Galactic center -- Sun direction and a semimajor axis of no more than 3 kpc.
14 pages, 7 figures
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- Combined dynamical effects of the bar and spiral arms in a Galaxy model. Application to the solar neighbourhood
- The structure of the Milky Way based on unWISE 3.4m integrated photometry
- Hercules and Wolf 630 Stellar Streams and Galactic Bar Kinematics
- Three-dimensional decomposition of galaxies with bulge and long bar