Zobrazeno 1 - 10
of 19
pro vyhledávání: '"Jean-Claude Passy"'
Autor:
Maria Wirzberger, Anastasia Lado, Mike Prentice, Ivan Oreshnikov, Jean-Claude Passy, Adrian Stock, Falk Lieder
Publikováno v:
Scientific Reports, Vol 14, Iss 1, Pp 1-16 (2024)
Abstract Distractions are omnipresent and can derail our attention, which is a precious and very limited resource. To achieve their goals in the face of distractions, people need to regulate their attention, thoughts, and behavior; this is known as s
Externí odkaz:
https://doaj.org/article/fd0e0866acca418890e4ca8eb6fe18bd
The effect of binding energy and resolution in simulations of the common envelope binary interaction
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 477:2349-2365
The common envelope binary interaction remains one of the least understood phases in the evolution of compact binaries, including those that result in Type Ia supernovae and in mergers that emit detectable gravitational waves. In this work we continu
The o80 C++ templated toolbox: Designing customized Python APIs for synchronizing realtime processes
Autor:
Manuel Wüthrich, Dieter Büchler, Maximilien Naveau, Vincent Berenz, Simon Guist, Felix Widmaier, Jean-Claude Passy
Publikováno v:
Journal of Open Source Software. 6:2752
Autor:
Dimitri Douchin, David J. Frew, Jean-Claude Passy, Michael T. Fitzgerald, George H. Jacoby, Maxwell Moe, D. Harmer, Orsola De Marco, G. Jasniewicz, Todd C. Hillwig
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 448:3132-3155
There is no conclusive explanation of why ∼80 per cent of planetary nebulae (PNe) are non-spherical. In the Binary Hypothesis, a binary interaction is a preferred channel to form a non-spherical PN. A fundamental step to corroborate or disprove the
The common envelope binary interaction occurs when a star transfers mass onto a companion that cannot fully accrete it. The interaction can lead to a merger of the two objects or to a close binary. The common envelope interaction is the gateway of al
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ed4dfe0bd36e2b995fadc2afeddb607f
Autor:
James Wurster, Roberto Iaconi, Thomas Reichardt, Jan E. Staff, Jean-Claude Passy, Daniel J. Price, Orsola De Marco, Falk Herwig
We present hydrodynamic simulations of the common envelope binary interaction between a giant star and a compact companion carried out with the adaptive mesh refinement code ENZO and the smooth particle hydrodynamics code PHANTOM. These simulations m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::568f09c67a378079dbbeec40d4cf2252
http://arxiv.org/abs/1603.01953
http://arxiv.org/abs/1603.01953
We present the results of hydrodynamic simulations of the interaction between a 10 Jupiter mass planet and a red or asymptotic giant branch stars, both with a zero-age main sequence mass of 3.5 $M_\odot$. Dynamic in-spiral timescales are of the order
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a25699ade3f3f8cec0cdf358c07e75b0
Autor:
Jean-Claude Passy, Mordecai-Mark Mac Low, Jeffrey S. Oishi, Falk Herwig, Chris L. Fryer, O. De Marco
Publikováno v:
Proceedings of the International Astronomical Union. 7:517-520
The common envelope interaction between a giant star and a stellar or substellar companion is at the origin of several compact binary classes, including the progenitors of Type Ia SN. A common envelope is also what will happen when the Sun expands an
Autor:
Jean-Claude Passy, Orsola De Marco, Falk Herwig, Maxwell Moe, Mordecai-Mark Mac Low, Bill Paxton
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 411:2277-2292
The {\alpha}-formalism is a common way to parametrize the common envelope interaction between a giant star and a more compact companion. The {\alpha} parameter describes the fraction of orbital energy released by the companion that is available to ej
Autor:
Roberto Iaconi, Pablo Galaviz, Mordecai-Mark Mac Low, Jean-Claude Passy, Orsola De Marco, Daniel Macdonald, Jan E. Staff
The Rotten Egg Nebula has at its core a binary composed of a Mira star and an A-type companion at a separation >10 au. It has been hypothesized to have formed by strong binary interactions between the Mira and a companion in an eccentric orbit during
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f03ece06e98ea4a313586fe7426764cc
http://arxiv.org/abs/1510.08429
http://arxiv.org/abs/1510.08429