Abstract
A series of dynamical models of the Galaxy is constructed assuming that the entire disk is near the gravitational-stability limit. This imposes constraints on the dynamical and kinematic parameters of the main subsystems (the disk, bulge, and halo). The disk surface density in the solar neighborhood should not exceed 58 M ⊙/pc2. Further, we find that the observed local decrease in the rotational velocity at 6 kpc ≲ r ≲ 10 kpc is not associated with details of the radial distribution of matter in the Galaxy and instead results from dynamical processes or some other factors responsible for noncircular motions. It follows from the presence of a long-lived bar and the observed distribution of the stellar-velocity dispersion that the central maximum in the rotation curve at radius r ⋍ 300 pc cannot be associated with a very concentrated bulge core. The best agreement between the observational data and the parameters of the dynamical models is achieved for a radial disk scale length of L ⋍ 3 kpc. The relative contribution of the disk to the circular rotational velocity at r = 2.2L is 73%.
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References
D. P. Clemens, Astrophys. J. 295, 422 (1985).
J. R. Lewis and K. C. Freeman, Astron. J. 97, 139 (1989).
J. Brand and L. Blitz, Astron. Astrophys. 275, 67 (1993).
Y. Sofue, Astrophys. J. 458, 120 (1996).
A. S. Rastorguev, E. V. Glushkova, A. K. Dambis, and M. V. Zabolotskikh, Pis’ma Astron. Zh. 25, 689 (1999) [Astron. Lett. 25, 595 (1999)].
Y. Sofue, Y. Tutui, M. Honma, et al., Astrophys. J. 523, 136 (1999).
T. C. Beers and J. Sommer-Larsen, Astrophys. J., Suppl. Ser. 96, 175 (1995).
M. Schmidt, Stars Stell. Syst. 4, 513 (1965).
J. A. R. Caldwell and J. P. Ostriker, Astrophys. J. 251, 61 (1981).
K. Rohlfs and J. Kreitsehmann, Astrophys. Space Sci. 79, 289 (1981).
B. Dauphole and J. Colin, Astron. Astrophys. 300, 117 (1995).
R. P. Olling and M. R. Merrifield, Mon. Not. R. Astron. Soc. 311, 361 (2000).
A. Toomre, Astrophys. J. 139, 1217 (1964).
A. G. Morozov and A. V. Khoperskov, Astrofizika 24, 467 (1986).
V. L. Polyachenko, E. V. Polyachenko, and A. V. Strel’nikov, Pis’ma Astron. Zh. 23, 598 (1997) [Astron. Lett. 23, 525 (1997)].
A. V. Khoperskov, A. V. Zasov, and N. V. Tyurina, Astron. Zh. 78, 213 (2001) [Astron. Rep. 45, 180 (2001)].
V. L. Polyachenko and I. G. Shykhman, Pis’ma Astron. Zh. 3, 254 (1977) [Sov. Astron. Lett. 3, 134 (1977)].
A. V. Zasov, D. I. Makarov, and E. A. Mikhailova, Pis’ma Astron. Zh. 17, 884 (1991) [Sov. Astron. Lett. 17, 374 (1991)].
A. G. Morozov, Astron. Zh. 58, 734 (1981) [Sov. Astron. 25, 421(1981)].
J. N. Bahcall and R. M. Soneira, Astrophys. J., Suppl. Ser. 44, 73 (1980).
A. A. Sumin, A. M. Fridman, and U. A. Khaud, Pis’ma Astron. Zh. 17, 698 (1991) [Sov. Astron. Lett. 17, 295 (1991)].
P. D. Sackett, Astrophys. J. 483, 103 (1997).
A. A. Sumin, A. M. Fridman, and U. A. Khaud, Pis’ma Astron. Zh. 17, 779 (1991) [Sov. Astron. Lett. 17, 329 (1991)].
R. Fux, Astron. Astrophys. 327, 983 (1997).
R. Fux, Astrophys. Space Sci. 276, 367 (2001).
W. Dehnen and J. J. Binney, Mon. Not. R. Astron. Soc. 298, 387 (1998).
J. N. Bahcall, Astrophys. J. 276, 156 (1984).
J. E. Barnes and P. Hut, Astrophys. J., Suppl. Ser. 70, 389 (1989).
A. M. Fridman, O. V. Khoruzhii, and A. E. Piskunov, in Physics of the Gaseous and Stellar Disks of the Galaxy, ASP Conf. Ser. 66, Ed. by I. R. King (Astronomical Society of the Pacific, San Francisco, 1994), p. 215.
A. C. Quillen and D. R. Garnett, in Galaxy Disks and Disk Galaxies, ASP Conf. Ser. 230, Ed. by J. G. Funes and S. J. Corsini (Astronomical Society of the Pacific, San Francisco, 2001), p. 87; astro-ph/0004210.
E. A. Mikhailova, A. V. Khoperskov, and S. S. Sharpak, in Stellar Dynamics: From Classic to Modern, Ed. by L. P. Ossipkov and I. I. Nikiforov (St. Petersburg, 2001), p. 147.
L. H. Amaral, R. Ortiz, J. R. D. Lepine, and W. J. Maciel, Mon. Not. R. Astron. Soc. 281, 339 (1996).
A. K. Dambis, A. M. Mel’nik, and A. S. Rastorguev, Pis’ma Astron. Zh. 21, 331 (1995) [Astron. Lett. 21, 291 (1995)].
I. I. Nikiforov, in Stellar Dynamics: From Classic to Modern, Ed. by L. P. Ossipkov and I. I. Nikiforov (St. Petersburg, 2001), p. 28.
A. K. Dambis, A. M. Mel’nik, and A. S. Rastorguev, Pis’ma Astron. Zh. 27, 68 (2001) [Astron. Lett. 27, 58 (2001)].
A. S. Rastorguev, M. V. Zabolotskikh, and A. K. Dambis, Astron. Lett. 28, 454 (2002).
I. I. Nikiforov, IAU Coll. 174: Small Galaxy Groups, ASP Conf. Ser. 209, Ed. by M. J. Valtonen and C. Flynn (Astronomical Society of the Pacific, San Francisco, 2000), p. 403.
P. C. van der Kruit and L. Searle, Astron. Astrophys. 95, 116 (1981).
P. C. van der Kruit, in Galaxy Disks and Disk Galaxies, ASP Conf. Ser. 230, Ed. by J. G. Funes and E. M. Corsini (Astronomical Society of the Pacific, San Francisco, 2001), p. 119.
A. V. Barabanov and A. V. Zasov, Astron. Zh. 56, 252 (1979) [Sov. Astron. 23, 138 (1979)].
A. M. N. Ferguson and C. J. Clarke, Mon. Not. R. Astron. Soc. 325, 781 (2001).
W. Dehnen, Astron. J. 115, 2384 (1998).
S. Frink, B. Fuchs, S. Roser, and R. Wiellen, Astron. Astrophys. 314, 430 (1996).
H. Hasan and C. Norman, Astrophys. J. 361, 69 (1990).
R. D. Blum, J. S. Carr, D. L. DePoy, et al., Astrophys. J. 422, 111 (1994).
R. D. Blum, J. S. Carr, K. Sellgren, and D. M. Terndrup, Astrophys. J. 449, 623 (1995).
R. M. Rich, Astrophys. J. 362, 604 (1990).
D. Minniti, S. D. M. White, E. W. Olszewski, and J. M. Hill, Astrophys. J. 393, L47 (1992).
K. Z. Stanek, A. Udalski, M. Szymaski, et al., Astrophys. J. 477, 163 (1997).
B. J. Weiner and J. A. Sellwood, Astrophys. J. 524, 112 (1999).
O. E. Gerhard, in Galaxy Disks and Disk Galaxies, Ed. by J. G. Funes and E. M. Corsini (Astron. Soc. of the Pacific, San Francisco, 2001), p. 21.
J. Binney, O. Gerhard, and D. Spergel, Mon. Not. R. Astron. Soc. 288, 365 (1997).
A. M. Fridman, in Physics of the Gaseous and Stellar Disks of the Galaxy, ASP Conf. Ser. 66, Ed. by I. R. King (Astronomical Society of the Pacific, San Francisco, 1994), p. 15.
T. J. Jones, M. Ashley, A. R. Hyland, and A. Ruelas-Mayorga, Mon. Not. R. Astron. Soc. 197, 413 (1981).
S. M. Kent, T. M. Dame, and G. Fazio, Astrophys. J. 378, 131 (1991).
R. Fux and L. Martinet, Astron. Astrophys. 287, L21 (1994).
H. T. Freudenreich, Astrophys. J. 492, 495 (1998).
P. L. Hammersley, M. Cohen, F. Garzon, et al., Mon. Not. R. Astron. Soc. 308, 333 (1999).
J. N. Bahcall and S. Casertano, Astrophys. J. 284, L35 (1984).
A. Gould, Mon. Not. R. Astron. Soc. 244, 25 (1990).
K. Kuijken and G. Gilmore, Astrophys. J. Lett. 367, L9 (1991).
M. Creze, E. Chereul, O. Bienayme, and C. Pichon, Astron. Astrophys. 329, 920 (1998).
A. Could, J. N. Bahcall, and C. Flynn, Astrophys. J. 465, 759 (1996).
N. I. Reid and S. R. Majewski, Astrophys. J. 409, 635 (1993).
M. Haywood, A. C. Robin, and M. Creze, Astron. Astrophys. 320, 440 (1997).
A. Vallenari, G. Bertelli, and L. Schmidtobreick, Astron. Astrophys. 361, 73 (2000).
C. Alard, Mon. Not. R. Astron. Soc. (2001); astro-ph/0007013.
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 80, No. 6, 2003, pp. 483–498.
Original Russian Text Copyright © 2003 by Khoperskov, Tyurina.
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Khoperskov, A.V., Tyurina, N.V. A dynamical model of the Galaxy. Astron. Rep. 47, 443–457 (2003). https://doi.org/10.1134/1.1583771
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DOI: https://doi.org/10.1134/1.1583771