COSMIC GAS-DYNAMICS, WHY WAS IT SO DIFFICULT

[1] [Anonymous], 1946, MON NOT R ASTRON SOC, V106, P159

[2] AXFORD WI, 1960, PHILOS T R SOC A, V253, P301

[3] BLOEMEN H, 1991, INTERSTELLAR DISK HA

[4] BURGERS JM, 1956, ERVARING CONCEPTIE

[5] GOLDSWORTHY FA, 1960, PHILOS T R SOC A, V253, P277

[6] HOLT S, 1993, BACK GALAXY

[7] Lowan A.N, 1949, SCRIPTA MATH, V15, P33

[8] SHOCK-WAVE STRUCTURE IN THE CYNGUS LOOP [J]. ASTROPHYSICS AND SPACE SCIENCE, 1994, 216 (1-2) : 303 - 309

[9] WALLER WH, 1993, WORMS FROTH FINE SCA

[10] WIERINGA M, 1991, 327 MHZ STUDIES HIGH

[1] [Anonymous], 1946, MON NOT R ASTRON SOC, V106, P159

[2] AXFORD WI, 1960, PHILOS T R SOC A, V253, P301

[3] BLOEMEN H, 1991, INTERSTELLAR DISK HA

[4] BURGERS JM, 1956, ERVARING CONCEPTIE

[5] GOLDSWORTHY FA, 1960, PHILOS T R SOC A, V253, P277

[6] HOLT S, 1993, BACK GALAXY

[7] Lowan A.N, 1949, SCRIPTA MATH, V15, P33

[8] SHOCK-WAVE STRUCTURE IN THE CYNGUS LOOP [J]. ASTROPHYSICS AND SPACE SCIENCE, 1994, 216 (1-2) : 303 - 309

[9] WALLER WH, 1993, WORMS FROTH FINE SCA

[10] WIERINGA M, 1991, 327 MHZ STUDIES HIGH