Abstract
A series of numerical N-body simulations is performed in order to dynamically model the properties of four galaxies (NGC 5603, NGC 3198, NGC 891, and NGC 1566) with known rotation curves, radial disk scales L, and velocity dispersions of old disk stars at various galactocentric distances r. Each model includes a three-dimensional collisionless disk and rigid spherical components, whose relative mass μ was treated as a free parameter that differed from simulation to simulation. The observed disk stellar velocity dispersions were assumed to be equal to or (in the general case) greater than the corresponding line-of-sight projections of the simulated values for the adopted μ after the initially unstable disk is heated and arrives at a steady state. A comparison of the simulated and observed rotational velocities and velocity dispersions provides evidence for “light” disks with μ≥2 in the disk (r<4L).
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References
T. S. van Albada, J. N. Bahcall, K. Begeman, and R. Sancisi, Astrophys. J. 295, 305 (1985).
S. M. Kent, Astron. J. 91, 1301 (1986).
P. Salucci and M. Persic, Astron. Astrophys. 351, 442 (1999).
A. V. Zasov, D. I. Makarov, and E. A. Mikhailova, Pis'ma Astron. Zh. 17, 884 (1991).
R. Bottema and J. P. E. Gerritsen, Mon. Not. R. Astron. Soc. 290, 585 (1997).
S. Courteau and H. Rex, Astrophys. J. 513, 561 (1999)).
B. Fuchs, in Galaxy Dynamics, Eds. by D. R. Merrit et al.; Astron. Soc. Pac. Conf. Ser. 182 (1999).
A. G. Morozov and A. V. Zasov, Astron. Zh. 62, 475 (1985) [Sov. Astron. 29, 277 (1985)].
A. V. Zasov, Pis'ma Astron. Zh. 11, 730 (1985) [Sov. Astron. Lett. 11, 307 (1985)].
E. A. Mikhailova and A. V. Khoperskov, Astron. Zh. 69, 1112 (1992) [Sov. Astron. 36, 573 (1992)].
R. Bottema, Astron. Astrophys. 275, 16 (1993).
E. Athanassoula, A. Bosma, and S. Papaioannou, Astron. Astrophys. 179, 23 (1987).
G. Efstathiou, G. Lake, and J. Negroponte, Mon. Not. R. Astron. Soc. 199, 1069 (1982).
J. C. Mihos, S. S. McGaugh, and W. J. G. de Block, Astrophys. J. Lett. 477, L79 (1997).
A. Toomre, Astrophys. J. 139, 1217 (1964).
J. A. Sellwood and R. G. Carlberg, Astrophys. J. 282, 61 (1984).
R. G. Carlberg and J. A. Sellwood, Astrophys. J. 292, 79 (1985).
J. M. Bardeen, in IAU Symposium 69: Dynamics of Stellar Systems, Ed. by A. Hayli (D. Reidel, Dordrecht, 1975), p. 297.
V. L. Polyachenko, E. V. Polyachenko, and A. V. Strel'nikov, Pis'ma Astron. Zh. 23(8), 598 (1997) [Astron. Lett. 23, 525 (1997)].
A. G. Morozov, Pis'ma Astron. Zh. 7, 197 (1981) [Sov. Astron. Lett. 7, 109 (1981)].
N. N. Gor'kavyi and A. M. Fridman, Physics of Planetary Rings [in Russian] (Nauka, Moscow, 1994).
A. G. Morozov, Astron. Zh. 58, 734 (1981) [Sov. Astron. 25, 421 (1981)].
R. Hockney and J. Eastwood, Computer Simulation Using Particles (McGraw-Hill, New York, 1984; Mir, Moscow, 1987).
J. P. Ostriker and P. J. E. Peebles, Astrophys. J. 186, 467 (1973).
A. G. Morozov, Astron. Zh. 58, 34 (1981) [Sov. Astron. 25, 19 (1981)].
K. G. Begeman, A. H. Broels, and R. H. Sanders, Mon. Not. R. Astron. Soc. 249, 523 (1991).
J. V. Villumsen, Astrophys. J. 290, 75 (1985).
P. C. van der Kruit and R. de Grijs, Astron. Astrophys. 352, 129 (1999).
Y. Sofue and N. Nakai, Publ. Astron. Soc. Jpn. 45, 139 (1993).
R. Bottema, P. C. van der Kruit, and E. A. Valentijn, Astron. Astrophys. 247, 357 (1991).
R. C. Kennicutt, Astron. J. 86, 1847 (1981).
R. Bottema, Astron. Astrophys. 257, 69 (1992).
Y. I. Byun, N. D. Kylafis, E. V. Paleologou, et al., Astron. Astrophys. 344, 868 (1999).
V. L. Polyachenko and I. G. Shukhman, Pis'ma Astron. Zh. 3, 254 (1977) [Sov. Astron. Lett. 3, 134 (1977)].
P. C. van der Kruit and L. Searle, Astron. Astrophys. 95, 105 (1981).
V. L. Polyachenko, Pis'ma Astron. Zh. 3, 99 (1977) [Sov. Astron. Lett. 3, 51 (1977)].
A. G. Morozov, Pis'ma Astron. Zh. 9, 716 (1983) [Sov. Astron. Lett. 9, 370 (1983)].
G. de Vaucouleurs, A. de Vaucouleurs, H. Corwin, et al., Third Reference Catalogue of Galaxies (Springer-Verlag, New York, 1991).
W. D. Pence and P. Taylor, Astrophys. J. 357, 415 (1990).
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 78, No. 3, 2001, pp. 213–228.
Original Russian Text Copyright © 2001 by Khoperskov, Zasov, Tyurina.
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Khoperskov, A.V., Zasov, A.V. & Tyurina, N.V. Estimating the masses of the spherical and disk components of galaxies via numerical simulations. Astron. Rep. 45, 180–194 (2001). https://doi.org/10.1134/1.1353358
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DOI: https://doi.org/10.1134/1.1353358