activity
20022026
most citedAccelerating infall and rotational spin-up in the hot molecular core G31.41+0.31

69 citations · 213 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2026

ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves

Tim Dietrich, Tanja Hinderer, Micaela Oertel +40

Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…

physics.bio-ph2022★ 1 cited

Muscle pre-stimulation tunes viscous-like perturbation rejection in legged hopping

Fabio Izzi, An Mo, Syn Schmitt +2

Muscle fibres possess unique visco-elastic properties, capable of generating a stabilising zero-delay response to unexpected perturbations. This instantaneous response -- termed "p…

astro-ph.EP2019★ 29 cited

Realistic collisional water transport during terrestrial planet formation: Self-consistent modeling by an N-body--SPH hybrid code

C. Burger, Á. Bazsó, C. M. Schäfer

According to current evidence the water inventory of Earth (and perhaps similar exoplanets) was transported inwards via (giant) collisions during the chaotic final phase of planet…

astro-ph.SR2018★ 69 cited

Accelerating infall and rotational spin-up in the hot molecular core G31.41+0.31

M. T. Beltrán, R. Cesaroni, V. M. Rivilla +20

As part of our effort to search for circumstellar disks around high-mass stellar objects, we observed the well-known core G31.41+0.31 with ALMA at 1.4 mm with an angular resolution…

astro-ph.HE2015★ 11 cited

Properties and observability of glitches and anti-glitches in accreting pulsars

L. Ducci, P. M. Pizzochero, V. Doroshenko +3

Several glitches have been observed in young, isolated radio pulsars, while a clear detection in accretion-powered X-ray pulsars is still lacking. We use the Pizzochero snowplow mo…

astro-ph.HE2012★ 53 cited

The runaway instability in general relativistic accretion disks

O. Korobkin, E. Abdikamalov, N. Stergioulas +4

When an accretion disk falls prey to the runaway instability, a large portion of its mass is devoured by the black hole within a few dynamical times. Despite decades of effort, it…