Zobrazeno 1 - 10
of 114
pro vyhledávání: '"Reichardt, Thomas"'
Autor:
Baker, A. Makai, Lasky, Paul D., Thrane, Eric, Ashton, Gregory, Cantos, Jesmigel, Lakerink, Lewis, Leslie, Asher, Poole, Gregory B., Reichardt, Thomas
There are at present ${\cal O}(100)$ gravitational-wave candidates from compact binary mergers reported in the astronomical literature. As detector sensitivities are improved, the catalog will swell in size: first to ${\cal O}(1000)$ events in the A+
Externí odkaz:
http://arxiv.org/abs/2204.13267
We study the formation of dust in the expanding gas ejected as a result of a common envelope binary interaction. In our novel approach, we apply the dust formation model of Nozawa et al. to the outputs of the 3D hydrodynamic SPH simulation performed
Externí odkaz:
http://arxiv.org/abs/2003.06151
Autor:
Zou, Yangyuxin, Frank, Adam, Chen, Zhuo, Reichardt, Thomas, De Marco, Orsola, Blackman, Eric G., Nordhaus, Jason, Balick, Bruce, Carroll-Nellenback, Jonathan, Chamandy, Luke, Liu, Baowei
The morphology of bipolar planetary nebulae (PNe) can be attributed to interactions between a fast wind from the central engine and dense toroidal shaped ejecta left over from common envelope (CE) evolution. Here we use the 3-D hydrodynamic AMR code
Externí odkaz:
http://arxiv.org/abs/1912.01647
Publikováno v:
In Annals of Nuclear Energy November 2023 192
During the common envelope binary interaction, the expanding layers of the gaseous common envelope recombine and the resulting recombination energy has been suggested as a contributing factor to the ejection of the envelope. In this paper we perform
Externí odkaz:
http://arxiv.org/abs/1911.02759
We present 1D-MESA2HYDRO-3D, an open source, Python-based software tool that provides an accessible means of generating physically motivated initial conditions (ICs) for hydrodynamical simulations from 1-D stellar structure models. We test 1D-MESA2HY
Externí odkaz:
http://arxiv.org/abs/1907.09062
We investigate the common envelope binary interaction, that leads to the formation of compact binaries, such as the progenitor of Type Ia supernovae or of mergers that emit detectable gravitational waves. In this work we diverge from the classic nume
Externí odkaz:
http://arxiv.org/abs/1907.03980
Autor:
Reichardt, Thomas A., De Marco, Orsola, Iaconi, Roberto, Tout, Christopher A., Price, Daniel J.
We have simulated a common envelope interaction of a 0.88-M$_{\odot}$, 90-R$_{\odot}$, red giant branch star and a 0.6-M$_{\odot}$, compact companion with the smoothed particle hydrodynamics code, Phantom, from the beginning of the Roche lobe overflo
Externí odkaz:
http://arxiv.org/abs/1809.02297
Autor:
Frank, Adam, Chen, Zhuo, Reichardt, Thomas, De Marco, Orsola, Blackman, Eric, Nordhaus, Jason
The morphologies of planetary nebula have long been believed to be due to wind shaping processes in which a fast wind from the central star impacts a previously ejected envelope. Asymmetries assumed to exist in the slow wind envelope lead to inertial
Externí odkaz:
http://arxiv.org/abs/1807.05925
Autor:
Eaton, Samuel W., Cárdenas, Edna S., Hix, Jay D., Johnson, James T., Watson, Scott M., Chichester, David L., Garcés, Milton A., Magaña-Zook, Steven A., Maceira, Monica, Marcillo, Omar E., Chai, Chengping, d'Entremont, Brian P., Reichardt, Thomas A.
Publikováno v:
In Applied Acoustics October 2022 199