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SELF-SIMILAR COLLAPSE IN NEBULAR DISK AND THE TITIUS-BODE LAW
LI, XQ ; ZHANG, H ; LI, QB
1995
Source PublicationASTRONOMY AND ASTROPHYSICS
ISSN0004-6361
Volume304Issue:2Pages:617—621
AbstractNonlinear development and evolution of density disturbances in nebular disk are examined on the basis of our previous study(Li & Zhang 1994). It is shown that the perturbed density is unstable with respect to self-modulation, leading to the formation of the density field localization; in the nonlinear stage of the instability, development of the localized field will lead to collapse. For the case of self-similar collapse, perturbed density inially increases with time and then tends to form of steady rings with very large but limit amplitudes; and their distances r(n) from the center form a geometric progression, which is similar to the Titius-Bode law.
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/8477
Collection期刊(老文献)
Recommended Citation
GB/T 7714
LI, XQ,ZHANG, H,LI, QB. SELF-SIMILAR COLLAPSE IN NEBULAR DISK AND THE TITIUS-BODE LAW[J]. ASTRONOMY AND ASTROPHYSICS,1995,304(2):617—621.
APA LI, XQ,ZHANG, H,&LI, QB.(1995).SELF-SIMILAR COLLAPSE IN NEBULAR DISK AND THE TITIUS-BODE LAW.ASTRONOMY AND ASTROPHYSICS,304(2),617—621.
MLA LI, XQ,et al."SELF-SIMILAR COLLAPSE IN NEBULAR DISK AND THE TITIUS-BODE LAW".ASTRONOMY AND ASTROPHYSICS 304.2(1995):617—621.
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