Zobrazeno 1 - 10
of 256
pro vyhledávání: '"Murray, James R."'
Publikováno v:
In The Knee June 2024 48:63-75
Autor:
Bruce, David J., Hassaballa, Mohammed, Robinson, James R., Porteous, Andrew J., Murray, James R., Newman, John H.
Publikováno v:
In The Knee June 2020 27(3):1018-1027
Publikováno v:
MNRAS, Volume 401, Number 2, January 2010, pp. 1275-1289(15)
We present three dimensional smoothed particle hydrodynamics (SPH) calculations of irradiation-driven warping of accretion discs. Initially unwarped planar discs are unstable to the radiation reaction when the disc is illuminated by a central radiati
Externí odkaz:
http://arxiv.org/abs/1001.1520
Autor:
Smith, Amanda J., Haswell, Carole A., Murray, James R., Truss, Michael R., Foulkes, Stephen B.
Publikováno v:
Mon.Not.Roy.Astron.Soc.378:785-800,2007
(Abridged) We use 3D SPH calculations with higher resolution, as well as with more realistic viscosity and sound-speed prescriptions than previous work to examine the eccentric instability which underlies the superhump phenomenon in semi-detached bin
Externí odkaz:
http://arxiv.org/abs/0704.1519
Publikováno v:
Mon.Not.Roy.Astron.Soc. 366 (2006) 1399-1409
We present three dimensional smoothed particle hydrodynamics (SPH) calculations of warped accretion discs in X-ray binary systems. Geometrically thin, optically thick accretion discs are illuminated by a central radiation source. This illumination ex
Externí odkaz:
http://arxiv.org/abs/astro-ph/0601126
We compare the accretion flow onto the neutron star induced by Roche lobe overflow with that by the overflow from the Be disk, in a zero eccentricity, short period binary with the same mass transfer rate, performing three-dimensional Smoothed Particl
Externí odkaz:
http://arxiv.org/abs/astro-ph/0511529
Autor:
Barrière-Fouchet, Laure, Gonzalez, Jean-François, Murray, James R., Humble, Robin J., Maddison, Sarah T.
Publikováno v:
Astron.Astrophys.443:185,2005
We present the results of a three dimensional, locally isothermal, non-self-gravitating SPH code which models protoplanetary disks with two fluids: gas and dust. We ran simulations of a 1 Msun star surrounded by a 0.01 Msun disk comprising 99% gas an
Externí odkaz:
http://arxiv.org/abs/astro-ph/0508452
Autor:
Barriere-Fouchet, Laure, Gonzalez, Jean-Francois, Humble, Robin J., Maddison, Sarah T., Murray, James R.
We present the results of three-dimensional numerical simulations that include the effects of hydrodynamical forces and gas drag upon an evolving dusty gas disk. We briefly describe a new parallel, two phase numerical code based upon the smoothed par
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310909