431 citations · 1k across the 11 of their papers we have counts for
12 papers
GWCloud: a searchable repository for the creation and curation of gravitational-wave inference results
A. Makai Baker, Paul D. Lasky, Eric Thrane +6
There are at present gravitational-wave candidates from compact binary mergers reported in the astronomical literature. As detector sensitivities are improved, the…
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…
Bipolar Planetary Nebulae from Outflow Collimation by Common Envelope Evolution
Yangyuxin Zou, Adam Frank, Zhuo Chen +8
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 comm…
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…
Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
Meridith Joyce, Lianne Lairmore, Daniel J. Price +2
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 hydrodynam…
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…
Planetary Nebulae Shaped By Common Envelope Evolution
Adam Frank, Zhuo Chen, Thomas Reichardt +3
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. A…
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…
Post-common envelope PN, fundamental or irrelevant?
Orsola De Marco, T. Reichardt, R. Iaconi +6
One in 5 planetary nebulae are ejected from common envelope binary interactions but Kepler Space Telescope results are already showing this proportion to be larger. Their propertie…
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…
Insights Into the High-Energy Gamma-ray Emission of Markarian 501 from Extensive Multifrequency Observations in the Fermi Era
LAT collaboration, A. A. Abdo et al., the MAGIC collaboration +6
We report on the gamma-ray activity of the blazar Mrk 501 during the first 480 days of Fermi operation. We find that the average LAT gamma-ray spectrum of Mrk 501 can be well descr…