activity
20182020
collaborators

6 papers

astro-ph.SR2020

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…

astro-ph.SR2019

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…

astro-ph.SR2019

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…

astro-ph.SR2019

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…

astro-ph.SR2019

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…

astro-ph.SR2018

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…