Electronic Resource
Springer
Astrophysics and space science
216 (1994), S. 347-351
ISSN:
1572-946X
Keywords:
gas dynamics
;
galactic disks
;
bar instability
;
nuclear activity
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract Numerical simulations of two-component (stars + gas) self-gravitating galactic disks show that the interstellar gas can significantly affect the dynamical evolution of the disk even if its mass fraction (relative to the total galaxy mass) is as low as several percent. Aided by efficient energy dissipation, the gas becomes gravitationally unstable onlocal scale and forms massive clumps. Gravitational scattering of stars by these clumps leads to suppression of bar instability usually seen in heavy stellar disks. In this case, gas inflow towards the galactic center is driven by dynamical friction which gas clumps suffer instead of bar forcing.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00982516
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