Zobrazeno 1 - 10
of 112
pro vyhledávání: '"Warren, M S"'
Autor:
Kegerreis, J. A., Teodoro, L. F. A., Eke, V. R., Massey, R. J., Catling, D. C., Fryer, C. L., Korycansky, D. G., Warren, M. S., Zahnle, K. J.
Publikováno v:
ApJ 861 (2018) 52
We perform a suite of smoothed particle hydrodynamics simulations to investigate in detail the results of a giant impact on the young Uranus. We study the internal structure, rotation rate, and atmospheric retention of the post-impact planet, as well
Externí odkaz:
http://arxiv.org/abs/1803.07083
Publikováno v:
Astrophys.J.643:292-305,2006
We provide a description of the SNSPH code--a parallel 3-dimensional radiation hydrodynamics code implementing treecode gravity, smooth particle hydrodynamics, and flux-limited diffusion transport schemes. We provide descriptions of the physics and p
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512532
Autor:
Fryer, C. L., Warren, M. S.
Publikováno v:
Astrophys.J.601:391-404,2004
In this paper, we present the results of 3-dimensional collapse simulations of rotating stars for a range of stellar progenitors. We find that for the fastest spinning stars, rotation does indeed modify the convection above the proto-neutron star, bu
Externí odkaz:
http://arxiv.org/abs/astro-ph/0309539
Publikováno v:
Astrophys.J. 594 (2003) 390-403
We present 3-dimensional SPH simulations of supernova explosions from 100 seconds to 1 year after core-bounce. By extending our modelling efforts to a 3-dimensional hydrodynamics treatment, we are able to investigate the effects of explosion asymmetr
Externí odkaz:
http://arxiv.org/abs/astro-ph/0301120
Autor:
Fryer, C. L., Warren, M. S.
We present the first complete 3-dimensional simulations of the core-collapse of a massive star from the onset of collapse to the resultant supernova explosion. We compare the structure of the convective instabilities that occur in 3-dimensional model
Externí odkaz:
http://arxiv.org/abs/astro-ph/0206017
Autor:
Frenk, C. S., White, S. D. M., Bode, P., Bond, J. R., Bryan, G. L., Cen, R., Couchman, H. M. P., Evrard, A. E., Gnedin, N., Jenkins, A., Khokhlov, A. M., Klypin, A., Navarro, J. F., Norman, M. L., Ostriker, J. P., Owen, J. M., Pearce, F. R., Pen, U. -L., Steinmetz, M., Thomas, P. A., Villumsen, J. V., Wadsley, J. W., Warren, M. S., Xu, G., Yepes, G.
Publikováno v:
Astrophys.J.525:554-582,1999
We have simulated the formation of an X-ray cluster in a cold dark matter universe using 12 different codes. The codes span the range of numerical techniques and implementations currently in use, including SPH and grid methods with fixed, deformable
Externí odkaz:
http://arxiv.org/abs/astro-ph/9906160
We propose a method to determine the cosmic mass density Omega from redshift-space distortions induced by large-scale flows in the presence of nonlinear clustering. Nonlinear structures in redshift space such as fingers of God can contaminate distort
Externí odkaz:
http://arxiv.org/abs/astro-ph/9701177
Publikováno v:
Proceedings: Biological Sciences, 1999 Aug 01. 266(1428), 1587-1592.
Externí odkaz:
https://www.jstor.org/stable/51715
Publikováno v:
Proceedings of the National Academy of Sciences of the United States of America, 1997 Feb . 94(4), 1069-1073.
Externí odkaz:
https://www.jstor.org/stable/41285
Publikováno v:
Oecologia, 1992 Jan 01. 92(4), 563-567.
Externí odkaz:
https://www.jstor.org/stable/4220203