Stability condition of the Kelvin-Helmholtz instability for the two-component protogalaxy

Publications of the Astronomical Society of Japan

Volumn 49, Issue 4, 1997, Pages 435-437

  Kamaya, Hideyuki ^a  

^a KYOTO UNIVERSITY   (Japan)

Author keywords

Galaxy: formation; Hydrodynamics; Interstellar: clouds; Interstellar: medium

Indexed keywords

COSMOLOGY;

CONDITION; GALAXY FORMATIONS; HOT GAS; INTERSTELLAR CLOUDS; INTERSTELLAR MEDIAS; KELVIN- HELMHOLTZ INSTABILITIES; PROTOGALAXIES; RICHARDSON; STABILITY CONDITION; TWO-COMPONENT;

STABILITY;

EID: 0031286755     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/49.4.435     Document Type: Article

References (9)

1. Aharonson V., Regev O., Shaviv N. 1994, ApJ 426, 621
2. Chandrasekhar S. 1961, Hydrodynamic and Hydromagnetic Stability (Clarendon Press, Oxford) §103
3. Draine B.T., Giuliani J.L. Jr 1984, ApJ 281, 690
4. Ferrara A., Shchekinov Yu. 1993, ApJ 417, 595
5. Ikeuchi S., Norman C. 1991, ApJ 375, 479
6. Kamaya H. 1996, ApJ 465, 769
7. Kamaya H. 1997, ApJ 474, 308
8. McKee C.F. 1995, in The Physics of the Interstellar Medium and Intergalactic Medium, ed A. Ferrara, C.F. McKee, C. Heiles, P.R. Shapiro, ASP Conf. Ser. 80, p292
9. Miyahata K., Ikeuchi S. 1995, PASJ 47, L37