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Constraining dynamical models with observational data

Published online by Cambridge University Press:  06 January 2014

Jo Bovy
Jo Bovy*
Affiliation:
Institute for Advanced Study, Einstein Drive, Princeton, NJ 08540, USA email: [email protected]
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Abstract

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The spatial distribution and kinematics of stars in the Milky Way are linked through the gravitational potential. Observations of the positions and velocities of stars can therefore be used to measure the mass distribution of the Milky Way. I review steady-state dynamical modeling approaches and illustrate their use in constraining the local matter distribution and the circular velocity curve from the kinematics of stellar tracers. In a few years, Gaia will increase the number of precise positions and velocities by multiple orders of magnitude. I describe some of the dynamical analyses that will be possible with the Gaia data and discuss some promising avenues for the optimal analysis of dynamical data.

Keywords

Galaxy: abundancesGalaxy: diskGalaxy: fundamental parametersGalaxy: generalGalaxy: kinematics and dynamicsGalaxy: stellar contentGalaxy: structureISM: kinematics and dynamicssolar neighborhood
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S298: Setting the scene for Gaia and LAMOST , May 2013 , pp. 185 - 194
Copyright
Copyright © International Astronomical Union 2014 

References

Adibekyan, V. Zh., Sousa, S. G., Santos, N. C., et al. 2012, Astron. Astrophys., 545, A32Google Scholar
Binney, J. J. 2010, Mon. Not. Roy. Astron. Soc., 401, 2318Google Scholar
Binney, J. J. 2012, Mon. Not. Roy. Astron. Soc., 426, 1328Google Scholar
Binney, J. J. & McMillan, P. 2011, Mon. Not. Roy. Astron. Soc., 413, 1889CrossRefGoogle Scholar
Binney, J. & Tremaine, S., 2008, Galactic Dynamics: Second Edition (Princeton University Press)Google Scholar
Binney, J. J., et al. 2009, Proceedings of Joint Discussion 5 at IAU XXVII, Rio de Janeiro, arXiv:0911.2661CrossRefGoogle Scholar
Blitz, L. & Spergel, D. N. 1991, Astrophys. J., 379, 631CrossRefGoogle Scholar
Bovy, J., Murray, I., & Hogg, D. W. 2010, Astrophys. J., 711, 1157CrossRefGoogle Scholar
Bovy, J., Rix, H.-W., Liu, C., et al. 2012a, Astrophys. J., 753, 148CrossRefGoogle Scholar
Bovy, J. & Tremaine, S. 2012, Astrophys. J., 756, 89Google Scholar
Bovy, J., Allende Prieto, C., Beers, T. C., et al. 2012b, Astrophys. J., 759, 131Google Scholar
Creze, M., Chereul, E., Bienaymé, O., & Pichon, C. 1998, Astron. Astrophys., 329, 920Google Scholar
Dehnen, W. 1998, Astron. J., 115, 2384Google Scholar
Gebhardt, K., Richstone, D., Kormendy, J., et al. 2000, Astrophys. J., 119, 1157Google Scholar
Fuhrmann, K. 2011, Mon. Not. Roy. Astron. Soc., 414, 2893Google Scholar
Holmberg, J. & Flynn, C. 2000, Mon. Not. Roy. Astron. Soc., 313, 209Google Scholar
Holmberg, J. & Flynn, C. 2004, Mon. Not. Roy. Astron. Soc., 352, 440Google Scholar
Jeans, J. H. 1915, Mon. Not. Roy. Astron. Soc., 76, 70Google Scholar
Kuijken, K. & Gilmore, G. 1989a, Mon. Not. Roy. Astron. Soc., 239, 571CrossRefGoogle Scholar
Kuijken, K. & Gilmore, G. 1989b, Mon. Not. Roy. Astron. Soc., 239, 605Google Scholar
Lin, C. C., Yuan, C., & Shu, F. H. 1969, Astrophys. J., 155, 721Google Scholar
Magorrian, J. 2013, Mon. Not. Roy. Astron. Soc., submittedGoogle Scholar
McMillan, P. & Binney, J. J. 2013, Mon. Not. Roy. Astron. Soc., in pressGoogle Scholar
Oort, J. H. 1932, Bull. Astron. Inst. Neth., 6, 249Google Scholar
Rix, H.-W. & Bovy, J. 2013, Astron. Astrophys. Rev., 21, 61Google Scholar
Rix, H.-W., de Zeeuw, P. T., Cretton, N., van der Marel, R. P., & Carollo, C. M. 1997, Astrophys. J., 488, 702Google Scholar
Rubin, V. C. & Ford, W. K. Jr. 1970, Astrophys. J., 159, 379Google Scholar
Schwarzschild, M. 1979, Astrophys. J., 232, 236Google Scholar
Stepanishchev, A. S. & Bobylev, V. V. 2013, Ast. L., 39, 185Google Scholar
Ting, Y.-S., Rix, H.-W., Bovy, J., & van de Ven, G. 2013, Mon. Not. Roy. Astron. Soc., in pressGoogle Scholar
Yanny, B., Rockosi, C., Newberg, H. J., et al. 2009, Astron. J., 137, 4377Google Scholar
Zhang, L., Rix, H.-W., van de Ven, G, Bovy, J., Liu, C., & Zhao, G. 2013, Astrophys. J., in pressGoogle Scholar
Zwicky, F. 1933, Helv. Phys. Acta 6, 110Google Scholar