When the primary star in a close binary system evolves into a giant and engulfs its
companion, its core and the companion temporarily orbit each other inside a common …

After the companion dynamically plunges through the primary's envelope, the two cores
remain surrounded by a common envelope and the decrease of the orbital period P orb …

At least one in five of all planetary nebulae are the product of a common envelope (CE)
interaction, where the companion in-spirals into the envelope of an asymptotic giant branch …

If the envelope of a massive star is not entirely removed during common envelope (CE)
interaction with an orbiting compact (eg, black hole (BH) or neutron star (NS)) companion …

We present small-scale 3D hydrodynamical simulations of the evolution of a 0.3 M⊙ main-
sequence (MS) star that launches two perpendicular jets within the envelope of a 0.88 M⊙ …

We are witnessing the dawn of gravitational wave (GW) astronomy. With currently available
detectors, observations are restricted to GW frequencies in the range between∼ 10 Hz and …

Understanding common envelope (CE) evolution is an outstanding problem in binary
evolution. Although the CE phase is not driven by gravitational wave (GW) emission, the …

It has long been speculated that jet feedback from accretion on to the companion during a
common envelope (CE) event could affect the orbital evolution and envelope unbinding …

We conduct a long-time-scale (d) 3D simulation of a common-envelope event with a red
giant and a main-sequence companion, using the moving-mesh hydrodynamic solver …

Many stars harbour multiplanet systems. As these stars expand late in their evolutions, the
innermost planet may be engulfed, leading to a common envelope (CE) event. Even if this is …