GALACTIC MODELS WITH VARIABLE SPIRAL STRUCTURE

[1] [Anonymous], 1967, J COMPUT PHYS, DOI DOI 10.1016/0021-9991(67)90056-3

[2] Clouds-in-clouds, clouds-in-cells physics for many-body plasma simulation (Reprinted from the Journal of Computational Physics, vol 3, pg 494-511, 1969) [J]. JOURNAL OF COMPUTATIONAL PHYSICS, 1997, 135 (02) : 141 - 148

[3] BROWNRIGG DRK, 1975, THESIS U READING

[4] Hockney R. W., 1970, Methods in computational physics. IX. Plasma physics, P135

[5] EFFECT OF POPULATION-II STARS AND 3-DIMENSIONAL MOTION ON SPIRAL STRUCTURE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1974, 167 (02) : 351 - +

[6] SUPPRESSION OF BAR INSTABILITY BY A MASSIVE HALO [J]. ASTRONOMICAL JOURNAL, 1976, 81 (01) : 30 - 36

[7] HOHL F, 1974, 241 C INT CTR NAT RE, P55

[8] HOHL F, 1970, R343 NASA TR

[9] JAMES RA, 1977, J COMP PHYS

[10] ON SPIRAL STRUCTURE OF DISK GALAXIES [J]. ASTROPHYSICAL JOURNAL, 1964, 140 (02) : 646 - &

[1] [Anonymous], 1967, J COMPUT PHYS, DOI DOI 10.1016/0021-9991(67)90056-3

[2] Clouds-in-clouds, clouds-in-cells physics for many-body plasma simulation (Reprinted from the Journal of Computational Physics, vol 3, pg 494-511, 1969) [J]. JOURNAL OF COMPUTATIONAL PHYSICS, 1997, 135 (02) : 141 - 148

[3] BROWNRIGG DRK, 1975, THESIS U READING

[4] Hockney R. W., 1970, Methods in computational physics. IX. Plasma physics, P135

[5] EFFECT OF POPULATION-II STARS AND 3-DIMENSIONAL MOTION ON SPIRAL STRUCTURE [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1974, 167 (02) : 351 - +

[6] SUPPRESSION OF BAR INSTABILITY BY A MASSIVE HALO [J]. ASTRONOMICAL JOURNAL, 1976, 81 (01) : 30 - 36

[7] HOHL F, 1974, 241 C INT CTR NAT RE, P55

[8] HOHL F, 1970, R343 NASA TR

[9] JAMES RA, 1977, J COMP PHYS

[10] ON SPIRAL STRUCTURE OF DISK GALAXIES [J]. ASTROPHYSICAL JOURNAL, 1964, 140 (02) : 646 - &