Zobrazeno 1 - 10
of 99
pro vyhledávání: '"Joel E. Tohline"'
Autor:
Juhan Frank, Joel E. Tohline, Jan E. Staff, Geoffrey C. Clayton, Chris L. Fryer, Patrick M. Motl, Wesley Even, Steven Diehl
Currently there is great interest in the outcomes and astrophysical implications of mergers of double degenerate binaries. In a commonly adopted approximation, the components of such binaries are represented by polytropes with an index n=3/2. We pres
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1fac7fa122b570e11d16c9d61662633
Autor:
Ravi Kumar Kopparapu, Joel E. Tohline
Publikováno v:
The Astrophysical Journal. 697:2089-2095
In an earlier investigation, we proposed population boundaries for both inspiralling and mass-transferring double white dwarf (DWD) systems in the distance independent "absolute" amplitude-frequency domain of the proposed space-based gravitational-wa
Publikováno v:
Computing in Science & Engineering. 11:68-73
A relatively simple, customized Python module that plugs smoothly into an otherwise standard workflow within VisTrails facilitates a quantitative analysis of complex fluid flows in simulations of merging binary stars.
Autor:
Joel E. Tohline
Publikováno v:
Computing in Science & Engineering. 9:76-81
From the perspective of a computational scientist who models astrophysical fluid flows, the author describes the successes and frustrations he's had with the development and use of scientific visualization techniques. A biased view toward the future
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
Autor:
Joel E. Tohline
Publikováno v:
Annual Review of Astronomy and Astrophysics. 40:349-385
▪ Abstract Although we have a general understanding of the manner in which individual stars form, our understanding of how binary stars form is far from complete. This is in large part due to the fact that the star formation process happens very qu
Autor:
Joel E. Tohline, Dominic Marcello
We present a numerical method for the study of double white dwarf (DWD) binary systems at the onset of super-Eddington mass transfer. We incorporate the physics of ideal inviscid hydrodynamical flow, Newtonian self-gravity, and radiation transport on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cea596177211f2dbd1bb2489ebc58ae2
Autor:
Joel E. Tohline, Konstantinos Voyages
Publikováno v:
The Astrophysical Journal. 555:524-531
We have identified an orthogonal curvilinear coordinate system (ξ1,ξ2,ξ3) for which surfaces of constant ξ1 exactly coincide with equipotential surfaces in the Kuzmin potential. The three principal coordinates are ξ1 ≡ [x2 + y2 + (a + |z|)2]1/
Autor:
Joel E. Tohline, Eric I. Barnes
Publikováno v:
The Astrophysical Journal. 551:80-102
In an effort to better understand the formation and evolution of barred galaxies, we have examined the properties of equatorial orbits in the effective potential of one model of a rapidly rotating, steady-state gas-dynamical bar that has been constru