Yi-Fang Chang 2007 Phys. Scr. 76 385 doi:10.1088/0031-8949/76/4/017
Yi-Fang Chang
Show affiliationsBased on the hydrodynamics and hydromagnetics of nebula, we discuss the formation of binary stars using the qualitative analysis theory of a nonlinear equation. The nonlinear interaction and rotation play very crucial roles. Moreover, the Lorenz model may be derived from the equations of the hydrodynamics, whose two wings in the Lorenz model form just the binary stars, while the linear equations form only a single star.
97.80.-d Binary and multiple stars
Issue 4 (2007)
Received 31 May 2006, accepted for publication 3 August 2007
Published 14 September 2007
Yi-Fang Chang 2007 Phys. Scr. 76 385
R Benini et al 2005 Class. Quantum Grav. 22 1483
Taichiro Takagi 2005 J. Phys. A: Math. Gen. 38 1961
S.P. Regan et al 1997 Nucl. Fusion 37 657
Aykutlu Dâna and Yoshihisa Yamamoto 2005 Nanotechnology 16 S125
H W Lee et al 1997 Class. Quantum Grav. 14 L53
B Aslan et al 2004 Semicond. Sci. Technol. 19 399
R M Ribeiro et al 2009 New J. Phys. 11 115002
E Samanidou et al 2007 Rep. Prog. Phys. 70 409
J D Barrow and T Clifton 2006 Class. Quantum Grav. 23 L1