Zobrazeno 1 - 10
of 110
pro vyhledávání: '"Sato, Jun'ichi"'
Publikováno v:
Astrophys.J.713:1350-1362,2010
The Standing Accretion Shock Instability (SASI) is commonly believed to be responsible for large amplitude dipolar oscillations of the stalled shock during core collapse, potentially leading to an asymmetric supernovae explosion. The degree of asymme
Externí odkaz:
http://arxiv.org/abs/0910.3953
Publikováno v:
Astrophys.J.694:833-841,2009
The physical processes involved in the advective-acoustic instability are investigated with 2D numerical simulations. Simple toy models, developped in a companion paper, are used to describe the coupling between acoustic and entropy/vorticity waves,
Externí odkaz:
http://arxiv.org/abs/0809.2303
We consider the effect of a supernova (SN) explosion in a very massive binary that is expected to form in a portion of Population III stars with the mass higher than 100$M_\odot$. In a Population III binary system, a more massive star can result in t
Externí odkaz:
http://arxiv.org/abs/0804.3346
We perform two-dimensional hydrodynamic simulation on the gas stripping by radiation drag from an interstellar cloud moving in uniform radiation fields. To properly include relativistic radiation drag, the radiation hydrodynamic equation is solved wi
Externí odkaz:
http://arxiv.org/abs/astro-ph/0407254
Publikováno v:
Mon.Not.Roy.Astron.Soc. 342 (2003) 593
Two-dimensional numerical simulations of an accretion flow in a close binary system are performed by solving the Euler equations with radiative transfer. In the present study, the specific heat ratio is assumed to be constant while radiative cooling
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304238
Publikováno v:
Astrophys.J.582:L67-L70,2003
We report the first measurement of genus curves for the two-dimensional mass map in the neighborhood of rich, X-ray luminous galaxy cluster MS1054-03 at z=0.83, reconstructed from weak lensing data obtained by Suprime-Cam on the prime focus of 8.2m S
Externí odkaz:
http://arxiv.org/abs/astro-ph/0211099
We apply the morphological descriptions of two-dimensional contour map, the so-called Minkowski functionals (the area fraction, circumference, and Euler characteristics), to the convergence field $\kappa(\bm{\theta})$ of the large-scale structure rec
Externí odkaz:
http://arxiv.org/abs/astro-ph/0104015
Publikováno v:
SAE Transactions, 2003 Jan 01. 112, 843-850.
Externí odkaz:
https://www.jstor.org/stable/44741316
Publikováno v:
In Proceedings of the Combustion Institute 2007 31(2):2133-2140