431 citations · 1.1k across the 12 of their papers we have counts for
12 papers
Jets in Common Envelopes: a low mass main sequence star in a red giant
Diego Lopez-Camara, Fabio De Colle, Enrique Moreno Mendez +2
We present small-scale three-dimensional hydrodynamical simulations of the evolution of a 0.3Msun main sequence star which launches two perpendicular jets within the envelope of a…
Properties of the post in-spiral common envelope ejecta II: dust formation
Roberto Iaconi, Keiichi Maeda, Takaya Nozawa +2
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…
The impact of recombination energy on simulations of the common envelope binary interaction
Thomas Reichardt, Orsola De Marco, Roberto Iaconi +1
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 contribu…
Properties of the post in-spiral common envelope ejecta I: dynamical and thermal evolution
Roberto Iaconi, Keiichi Maeda, Orsola De Marco +2
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 detecta…
Companion-launched jets and their effect on the dynamics of common envelope interaction simulations
Sagiv Shiber, Roberto Iaconi, Orsola De Marco +1
We conduct three-dimensional hydrodynamic simulations of the common envelope binary interaction and show that if the companion were to launch jets while interacting with the giant…
Speaking with one voice: simulations and observations discuss the common envelope parameter
Roberto Iaconi, Orsola De Marco
We present a comparative study between the results of most hydrodynamic simulations of the common envelope binary interaction to date and observations of post common envelope binar…
Extending Common Envelope Simulations from Roche Lobe Overflow to the Nebular Phase
Thomas A. Reichardt, Orsola De Marco, Roberto Iaconi +2
We have simulated a common envelope interaction of a 0.88-M, 90-R, red giant branch star and a 0.6-M, compact companion with the smoothed particle hyd…
The effect of binding energy and resolution in simulations of the common envelope binary interaction
Roberto Iaconi, Orsola De Marco, Jean-Claude Passy +1
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 mer…
Common envelope light-curves - I. grid-code module calibration
Pablo Galaviz, Orsola De Marco, Jean-Claude Passy +2
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 t…
Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
Daniel J. Price, James Wurster, Terrence S. Tricco +24
We present Phantom, a fast, parallel, modular and low-memory smoothed particle hydrodynamics and magnetohydrodynamics code developed over the last decade for astrophysical applicat…
The effect of a wider initial separation on common envelope binary interaction simulations
Roberto Iaconi, Thomas Reichardt, Jan Staff +5
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 a…
Hydrodynamic Simulations of the Interaction between an AGB Star and a Main Sequence Companion in Eccentric Orbits
Jan E. Staff, Orsola De Marco, Daniel Macdonald +4
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 inte…