Search results
Jump to navigation
Jump to search
Page title matches
- ...ppendix A of [http://adsabs.harvard.edu/abs/2009ApJS..184..248E Even & Tohline (2009)]. ...first to construct models of spherically symmetric stars using the [[User:Tohline/SR#Time-Independent_Problems|barotropic equation of state appropriate for a18 KB (2,627 words) - 15:34, 9 August 2019
Page text matches
- <font color="black">Detailed Force-Balance</font><br>([[User:Tohline/SphericallySymmetricConfigurations/SolutionStrategies#Spherically_Symmetric <font color="black">Virial Equilibrium</font><br>([[User:Tohline/SphericallySymmetricConfigurations/Virial#Virial_Equilibrium_of_Spherically7 KB (936 words) - 16:32, 24 September 2016
- ...free-energy expression and/or virial equilibrium constructs to analyze the structure and stability of spherically symmetric configurations. <li><font size="+1">⓪</font> [[User:Tohline/SphericallySymmetricConfigurations/Virial#Virial_Equilibrium_of_Spherically9 KB (1,245 words) - 01:11, 21 November 2016
- An updated/replacement ''Appendix/Images'' page can be found [[User:Tohline/Appendix/Images|here]]. ==Generated by Tohline or an Immediate Collaborator==60 KB (8,340 words) - 23:10, 28 February 2019
- As we have reviewed in an [[User:Tohline/SSC/Structure/WhiteDwarfs#Chandrasekhar_mass|accompanying discussion]], ...e derivation of <math>~M_3</math> is presented in Chapter ''XI'' of [[User:Tohline/Appendix/References#C67|Chandrasekhar (1967)]].20 KB (2,815 words) - 21:44, 10 August 2019
- ...sed hypertext book (H_Book) reviews what is presently understood about the structure, stability, and dynamical evolution of (Newtonian) self-gravitating fluids. ...ut, in addition, chapters are included that review what is known about the structure and stability of self-gravitating ''incompressible'' (uniform-density) flui51 KB (6,272 words) - 17:27, 28 May 2021
- ...e combination of physical constants in this expression resemble the [[User:Tohline/Appendix/Ramblings/Radiation/CodeUnits#Application_to_Unit_Conversion_Expre Now, based on the accompanying discussion of the [[User:Tohline/SSC/Structure/WhiteDwarfs#Chandrasekhar_mass|Chandrasekhar mass]],8 KB (1,373 words) - 13:47, 24 May 2011
- ...ine/Math/C_SpeedOfLight}}, {{User:Tohline/Math/C_GasConstant}}, and {{User:Tohline/Math/C_RadiationConstant}}, Dominic used the following code-unit ...sely — assuming pure helium, that is, a mean molecular weight {{User:Tohline/Math/MP_MeanMolecularWeight}} of 2 — since the Thompson cross-section36 KB (5,220 words) - 20:25, 12 August 2010
- This replaces an earlier [[User:Tohline/Appendix/Images2016Layout|''Appendix/Images2016Layout'']] wiki page. <td align="left" colspan="3">WIKI CHAPTER: [[User:Tohline/Preface#Preface|Preface]]</td>97 KB (13,666 words) - 17:22, 19 July 2020
- ...ion has the following properties; this model has been selected from [[User:Tohline/ThreeDimensionalConfigurations/RiemannStype#Table2|Table 2 of our accompany ...]; essentially the same diagram appears in §49 (p. 147) of [<b>[[User:Tohline/Appendix/References#EFE|<font color="red">EFE</font>]]</b>].615 KB (24,699 words) - 03:56, 14 June 2020