CONTINUUM HYDRODYNAMICAL EQUATIONS FOR MULTIPHASE ASTROPHYSICAL FLOWS

被引:14
作者
PISTINNER, S [1 ]
SHAVIV, G [1 ]
机构
[1] TECHNION ISRAEL INST TECHNOL,DEPT PHYS,IL-32000 HAIFA,ISRAEL
关键词
H-II REGIONS; HYDRODYNAMICS; ISM; JETS AND OUTFLOWS;
D O I
10.1086/173107
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a formalism for averaging mutually interacting multiphase hydrodynamical flows. Only averaging over space is discussed. The outcome of this formulation is a set of nonlinear first-order integrodifferential equations. We then apply the formalism to the problem of H I regions immersed in H II regions and obtain approximated equations. The H I regions are treated as a dilute suspension of fluid spheres immersed in H II continuum. The equations include terms and coefficients that have to be evaluated from a ''mesoscopic'' hydrodynamical theory. The hydrodynamics of the flow past a single cloud, which is defined here as the ''mesoscale'' of a ''fluid particle'' for the system under consideration should provide the input physics to the formalism presented here.
引用
收藏
页码:612 / 625
页数:14
相关论文
共 20 条
[1]  
Bear J., 1990, INTRO MODELING TRANS, P449, DOI 10.1007/978-94-009-1926-6_7
[2]   GLOBAL EFFECTS OF THERMAL CONDUCTION ON 2-PHASE MEDIA [J].
BEGELMAN, MC ;
MCKEE, CF .
ASTROPHYSICAL JOURNAL, 1990, 358 (02) :375-391
[3]   NUMERICAL STUDY OF A 2-FLUID HYDRODYNAMIC MODEL OF THE INTERSTELLAR-MEDIUM AND POPULATION I-STARS [J].
CHIANG, WH ;
PRENDERGAST, KH .
ASTROPHYSICAL JOURNAL, 1985, 297 (02) :507-530
[4]  
GATEZ T, 1987, AP J, V316, P530
[5]  
KEGEL WH, 1987, PHYSICAL PROCESSES I
[6]  
Landau LD., 1987, COURSE THEORETICAL P, V6
[7]  
LANGBEIN T, 1990, ASTRON ASTROPHYS, V227, P333
[8]   MOLECULAR GAS IN ELLIPTIC GALAXIES [J].
LEES, JF ;
KNAPP, GR ;
RUPEN, MP ;
PHILLIPS, TG .
ASTROPHYSICAL JOURNAL, 1991, 379 (01) :177-215
[9]   GALACTIC WINDS [J].
MATHEWS, WG ;
BAKER, JC .
ASTROPHYSICAL JOURNAL, 1971, 170 (02) :241-&
[10]   STEADY EVAPORATION AND CONDENSATION OF ISOLATED CLOUDS IN HOT PLASMA [J].
MCKEE, CF ;
BEGELMAN, MC .
ASTROPHYSICAL JOURNAL, 1990, 358 (02) :392-398