Hostname: page-component-cd9895bd7-jkksz Total loading time: 0 Render date: 2024-12-22T21:16:43.618Z Has data issue: false hasContentIssue false
  • English
  • Français

Kinematics of the Galactic Bulge from Radial Velocity and Proper Motion Optical Surveys

Published online by Cambridge University Press:  05 March 2013

Céline Reylé ,
Annie C. Robin  and
Sébastien Picaud
Céline Reylé*
Affiliation:
Observatoire de Besançon, BP 1615, 25010 Besançon Cedex, France
Annie C. Robin
Affiliation:
Observatoire de Besançon, BP 1615, 25010 Besançon Cedex, France
Sébastien Picaud
Affiliation:
Observatoire de Besançon, BP 1615, 25010 Besançon Cedex, France
*
2E-mail: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Large-scale surveys provide new constraints on the structure and evolution of the Milky Way. The population synthesis approach is a useful tool to interpret such data sets and to test scenarios of evolution of the Galaxy. New constraints on Galactic parameters have been obtained from the Besançon model of population synthesis, in particular in the inner regions, thanks to near-infrared surveys less affected by interstellar extinction than the optical ones. We present here a few preliminary comparisons between observed and simulated distributions of proper motions in the direction of the Galactic bulge. Next we discuss how bulge stars can be observed and separated from other populations with the RAVE and Gaia surveys.

Keywords

Galaxy: bulgeGalaxy: kinematics and dynamicssurveys
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 21 , Issue 2: The Fifth Workshop on Galactic Chemodynamics , 2004 , pp. 138 - 143
Copyright
Copyright © Astronomical Society of Australia 2004

References

Alard, C. 2003, A&A, preprint astro-ph/0306624Google Scholar
Høg, E. 2002, Gaia report GAIA-CUO-115Google Scholar
Ibata, R. A., & Gilmore, G. F. 1995, MNRAS, 275, 605 Google Scholar
Jordi, C., Figueras, F., Carrasco, J. M., & Knude, J. 2003, Gaia report UB-PWG-009Google Scholar
Minniti, D. 1996, ApJ, 459, 579 Google Scholar
Minniti, D., Liebert, J., Olszewski, E. W., & White, S. D. M. 1996, AJ, 112, 590 Google Scholar
Parker, Q. A., & Phillipps, S. 2001, in The New Era of Wide Field Astronomy, ASP Conf. Series 232, eds. R. Clowes, A. Adamson, & G. Bromage (San Francisco: ASP), 38 Google Scholar
Perryman, M. A. C. 2002, Ap&SS, 280, 1 Google Scholar
Peyaud, A. E., Parker, Q. A., Acker, A. A., & Bond, I. A. 2003, in White Dwarfs: Galactic and Cosmologic Probes, 25th meeting of the IAU, Joint Discussion 5, 16–17 July 2003, SydneyGoogle Scholar
Picaud, S., Chereul, E., Robin, A. C., & Garzón, F. 2003, Ap&SS, 284, 523 Google Scholar
Robin, A. C., Reylé, C., Derrière, S., & Picaud, S. 2003, A&A, 409, 523 Google Scholar
Schlegel, D. J., Finkbeiner, D. P., & Davis, M. 1998, ApJ, 500, 525 CrossRefGoogle Scholar
Schultheis, M., et al. 1999, A&A, 349, L69 Google Scholar
Steinmetz, M. 2003, in Gaia Spectroscopy, Science, and Technology, ASP Conf. Series 298, ed. U. Munari (San Francisco: ASP), 381 Google Scholar
Sumi, T., et al. 2004, MNRAS, 348, 1439 Google Scholar
Tiede, G. P., & Terndrup, D. M. 1999, AJ, 118, 895 Google Scholar