[HTML][HTML] Common envelope evolution: where we stand and how we can move forward
N Ivanova, S Justham, X Chen, O De Marco… - The Astronomy and …, 2013 - Springer
This work aims to present our current best physical understanding of common-envelope
evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas …
evolution (CEE). We highlight areas of consensus and disagreement, and stress ideas …
[HTML][HTML] Binary stars in the new millennium
Binary stars are as common as single stars. Binary stars are of immense importance to
astrophysicists because that they allow us to determine the masses of the stars independent …
astrophysicists because that they allow us to determine the masses of the stars independent …
A circumbinary disc in the final stages of common envelope and the core-degenerate scenario for Type Ia supernovae
We study the final stages of the common envelope (CE) evolution and find that a substantial
fraction of the ejected mass does not reach the escape velocity. To reach this conclusion we …
fraction of the ejected mass does not reach the escape velocity. To reach this conclusion we …
The origin and shaping of planetary nebulae: putting the binary hypothesis to the test
O De Marco - Publications of the Astronomical Society of the …, 2009 - iopscience.iop.org
Planetary nebulae (PNs) are circumstellar gas ejected during an intense mass-losing phase
in the lives of asymptotic giant branch stars. PNs have a stunning variety of shapes, most of …
in the lives of asymptotic giant branch stars. PNs have a stunning variety of shapes, most of …
The Hα surface brightness–radius relation: a robust statistical distance indicator for planetary nebulae
Measuring the distances to Galactic planetary nebulae (PNe) has been an intractable
problem for many decades. We have now established a robust optical statistical distance …
problem for many decades. We have now established a robust optical statistical distance …
A catalog of potential post–common envelope binaries
MU Kruckow, PG Neunteufel, R Di Stefano… - The Astrophysical …, 2021 - iopscience.iop.org
We present a catalog containing 839 candidate post–common envelope systems. Common
envelope evolution is very important in stellar astrophysics, particularly in the context of very …
envelope evolution is very important in stellar astrophysics, particularly in the context of very …
Binary planetary nebulae nuclei towards the Galactic bulge-I. Sample discovery, period distribution, and binary fraction
B Miszalski, A Acker, AFJ Moffat, QA Parker… - Astronomy & …, 2009 - aanda.org
Binarity has been hypothesised to play an important, if not ubiquitous, role in the formation of
planetary nebulae (PNe). Yet there remains a severe paucity of known binary central stars …
planetary nebulae (PNe). Yet there remains a severe paucity of known binary central stars …
Binary stars as the key to understanding planetary nebulae
D Jones, HMJ Boffin - Nature Astronomy, 2017 - nature.com
Planetary nebulae are traditionally considered to represent the final evolutionary stage of all
intermediate-mass stars (∼ 0.7–8 M☉). Recent evidence seems to contradict this picture. In …
intermediate-mass stars (∼ 0.7–8 M☉). Recent evidence seems to contradict this picture. In …
[HTML][HTML] Post common envelope binaries from SDSS-XII. The orbital period distribution
AN Gómez-Morán, BT Gänsicke, MR Schreiber… - Astronomy & …, 2011 - aanda.org
Context. The complexity of the common-envelope phase and of magnetic stellar wind
braking currently limits our understanding of close binary evolution. Because of their …
braking currently limits our understanding of close binary evolution. Because of their …
Simulations of common envelope evolution in triple systems: circumstellar case
The dynamical evolution of triple stellar systems could induce the formation of compact
binaries and binary mergers. Common envelope (CE) evolution, which plays a major role in …
binaries and binary mergers. Common envelope (CE) evolution, which plays a major role in …