Hydrostatic, isothermal planetary models from the point of view of dynamical systems: “Determination of explicit formulas for the point of critical mass”-Reference-Cited by-同舟云学术

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Hydrostatic, isothermal planetary models from the point of view of dynamical systems: “Determination of explicit formulas for the point of critical mass”

Published:2007-07 Issue:10 Volume:55 Page:1299-1309
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Schönke Johannes

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference14 articles.

1. Broeg, C., 2006. Dissertation, Universität Jena.

2. Hayashi, C., Nakazawa, K., Nakagawa, Y., 1985. Protostars and Planets II, p. 1100.

3. Formation of Giant Planets in Dense Nebulae: Critical Core Mass Revisited

4. Stellar Structure and Evolution;Kippenhahn,1990

5. Formation of the Giant Planets

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2. Planet masses and radii from physical principles;Proceedings of the International Astronomical Union;2010-10

3. The stability of ultra-compact planetary systems;Astronomy and Astrophysics;2010-06

4. The full set of gas giant structuresI: On the origin of planetary masses and the planetary initial mass function;Icarus;2009-11

5. STEADY STATES OF SELF-GRAVITATING INCOMPRESSIBLE FLUID WITH AXIAL SYMMETRY;International Journal of Modern Physics A;2009-09-20

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