Zobrazeno 1 - 10
of 12
pro vyhledávání: '"Shangli Ou"'
Publikováno v:
IAU Symposium 249. Cambridge: Cambridge University Press, 2008, pp.407-412
We use a multi-dimensional hydrodynamics code to study the gravitational interaction between an embedded planet and a protoplanetary disk with emphasis on the generation of vortensity (Potential Vorticity or PV) through a Baroclinic Instability. We s
Externí odkaz:
http://arxiv.org/abs/0805.3009
Autor:
Zachary Lawrence, Xiujun Yang, Lieve Vanneste, Daniel Eke, Vikas Gudipati, Shangli Ou, Alana P. Robinson, Brian deMartin, Gboyega Ayeni, Irina Gorysheva
Publikováno v:
First International Meeting for Applied Geoscience & Energy Expanded Abstracts.
Publikováno v:
SEG Technical Program Expanded Abstracts 2017.
Publikováno v:
SEG Technical Program Expanded Abstracts 2016.
Publikováno v:
The Astrophysical Journal. 667:1220-1228
We use a multi-dimensional hydrodynamics code to study the gravitational interaction between an embedded planet and a protoplanetary disk with emphasis on the generation of vortensity (potential vorticity) through a Baroclinic Instability and subsequ
Publikováno v:
Proceedings of the International Astronomical Union. 3:407-412
We use a multi-dimensional hydrodynamics code to study the gravitational interaction between an embedded planet and a protoplanetary disk with emphasis on the generation of vortensity (Potential Vorticity or PV) through a Baroclinic Instability. We s
Autor:
Joel E. Tohline, Shangli Ou
Publikováno v:
The Astrophysical Journal. 651:1068-1078
A one-armed spiral instability has been found to develop in differentially rotating stellar models that have a relatively stiff, $n=1$ polytropic equation of state and a wide range of rotational energies. This suggests that such instabilities can ari
Publikováno v:
The Astrophysical Journal. 617:490-499
We have modelled the nonlinear development of the secular bar-mode instability that is driven by gravitational radiation-reaction (GRR) forces in rotating neutron stars. In the absence of any competing viscous effects, an initially uniformly rotating
Publikováno v:
International Workshop on Gravity, Electrical & Magnetic Methods and Their Applications, Beijing, China, October 10–13, 2011.
Using a three-dimensional nonlinear hydrodynamic code, we examine the dynamical stability of more than twenty self-gravitating, compressible, ellipsoidal fluid configurations that initially have the same velocity structure as Riemann S-type ellipsoid
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f7836f49d61a6d6a92fa10630db486a