Evolution and dynamical stability of the proto-giant-planet envelope

Icarus

Volumn 126, Issue 2, 1997, Pages 282-292

  Tajima, Nobuya ^a   Nakagawa, Yoshitsugu ^b  

^a UNIVERSITY OF TOKYO   (Japan)

^b KOBE UNIVERSITY   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0031116844     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.1996.5651     Document Type: Article

References (37)

1. Baker N. Simplified models for cepheid instability. Stellar Evolution. 1966;Plenum, New York. p. 333-346.
2. Beckwith S. V. W., Sargent A. I., Chini R. S., Güsten R. A survey for circumstellar disks around young stellar objects. Astron. J. 99:1990;924-945.
3. Bodenheimer P. Evolution of the giant planets. Black D. C., Matthews M. S. Protostars and Planets II. 1985;873-894 Univ. of Arizona Press, Tucson.
4. Bodenheimer P., Pollack J. B. Calculations of the accretion and evolution of giant planets: The effects of solid cores. Icarus. 67:1986;391-408.
5. Chabrier G., Saumon D. The molecular-metallic transition of hydrogen and the structure of Jupiter and Saturn. Astrophys. J. 391:1992;817-826.
6. Cox J. P., Giuli R. T. Mixing length theory of convection. Principles of Stellar Structure: Physical Principles. 1968;Gordon and Breach, New York. p. 281-325.
7. Duffy T. S., Vos W. L., Zha C. S., Hemley R. J., Ho-kwang M. Sound velocities in dense hydrogen and the interior of Jupiter. Science. 263:1994;1590-1593.
8. Hayashi C. Structure of the solar nebula, growth and decay of magnetic fields and effects of magnetic and turbulent viscosities on the nebula. Prog. Theor. Phys. 70:1981;35-53.
9. Hayashi C., Nakazawa K., Nakagawa Y. Formation of the solar system. Black D. C., Matthews M. S. Protostars and Planets II. 1985;1100-1153 Univ. of Arizona Press, Tucson.
10. Landau E. D., Lifshitz E. M. Statical Physics Part I. 1988;Pergamon, New York.
11. Marley M. S., Hubbard W. B. Thermodynamics of dense molecular hydrogen-helium mixtures at high pressure. Icarus. 73:1988;536-544.
12. Miyake K., Nakagawa Y. Effects of particle size distribution on opacity curves of protoplanetary disks around T Tauri stars. Icarus. 106:1993;20-41.
13. Miyake K., Nakagawa Y. Dust particle settling in passive disks around T Tauri stars: Models andIRAS. Astrophys. J. 411:1995;361-384.
14. Mizuno H. Formation of the giant planets. Prog. Theor. Phys. 64:1980;544-557.
15. Mizuno H., Nakazawa K., Hayashi C. Instability of gaseous envelope surrounding planetary core and formation of giant planets. Prog. Theor. Phys. 60:1978;699-710.
16. Murai T., Sugimoto D., Hoshi R., Hayashi C. Evolution of carbon stars. I. Gravitational contraction and onset of carbon burning. Prog. Theor. Phys. 39:1968;619-634.
17. Nakagawa Y., Hayashi C., Nakazawa K. Accumulation of planetesimals in the solar nebula. Icarus. 54:1983;361-376.
18. Nellis W. J., Mitchell A. C., Van Thiel M., Devine G. J., Trainor R. J., Brown N. Equation of state data for molecular hydrogen and deuterium at shock pressures in the range 2-76 Gpa (20-760 kbar). J. Chem. Phys. 79:1983a;1480-1486.
19. Nellis W. J., Ross M., Mitchell A. C., Van Thiel M., Yung D. A., Ree F. H., Trainor R. J. Equation of state of molecular hydrogen and deuterium from shock wave experiments to 760 kbar. Phys. Rev. A. 27:1983b;608-611.
20. Podolak M., Hubbard W. B., Pollack J. B. Gaseous accretion and the formation of giant planets. Levy E. H., Lunine J. I. Protostars and Planets III. 1993;1109-1147 Univ. of Arizona Press, Tucson.
21. Pollack J. B., Podolak M., Bodenheimer P., Christofferson B. Planetesimal dissolution in the envelopes of the forming, giant planets. Icarus. 67:1986;409-443.
22. Saumon D., Chabrier G. Fluid hydrogen at high density: Pressure dissociation. Phys. Rev. A. 44:1991;5122-5141.
23. Saumon D., Chabrier G. Fluid hydrogen at high density: Pressure ionization. Phys. Rev. A. 46:1992;2084-2100.
24. Saumon D., Chabrier G., Van Horm H. M. An equation of state for low-mass stars and giant planet. Astrophys. J. Suppl. 99:1995;713-741.
25. Sekiya M., Miyama S. M., Hayashi C. Gas flow in the solar nebula leading to the formation of Jupiter. Earth, Moon, Planets. 39:1987;1-16.
26. Shu F. H. Mixing-length theory of convection. Osterbrock D. E., Miller J. S. The Physics of Astrophysics: Gas Dynamics. 1992;125-132 University Science Books, Mill Valley.
27. Shu F. H., Adams F. C., Lizano S. Star formation in molecular clouds: Observation and theory. Ann. Rev. Astron. Astrophys. 25:1987a;23-81.
28. Stahler S. W., Shu F. H., Taam R. E. The evolution of protostars. II. The hydrostatic core. Astrophys. J. 242:1980;226-241.
29. Stevenson D. J. Formation of the giant planets. Planet. Space Sci. 30:1982;755-764.
30. N. Tajima, 1994, Giant Planet Formation: The Dynamical Stability of the Envelope, University of Tokyo.
31. Tajima N., Nakagawa Y. Giant planet formation: The dynamical stability of a massive envelope. Earth, Moon, Planets. 67:1995;67-69.
32. Unno W., Osaki Y., Ando H., Saio H., Shibahasi H. Nonadiabatic oscillations. Nonradial Oscillations of Stars. 1989;Univ. of Tokyo Press, Tokyo. p. 209-232.
33. Wuchterl G. Hydrodynamics of giant planet formation. I. Overviewing the κ-mechanism. Astron. Astrophys. 238:1990;83-94.
34. Wuchterl G. Hydrodynamics of giant planet formation. II. Model equations and critical mass. Icarus. 91:1991a;39-52.
35. Wuchterl G. Hydrodynamics of giant planet formation. III. Jupiter's nucleated instability. Icarus. 91:1991b;53-64.
36. Wuchterl G. The critical mass for protoplanets revisited: Massive envelopes through convection. Icarus. 106:1993;323-334.
37. Wuchterl G. Giant planet formation: A comparative view of gas-accretion. Earth, Moon, Planets. 67:1995;51-65.