activity
20002025
most citedAccretion discs models with the "beta"-viscosity prescription derived from laboratory experiments

43 citations · 164 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.EP2025★ 3 cited

Edge-On Disk Study (EODS) III: Molecular Stratification in the Flying Saucer Disk

A. Dutrey, O. Denis-Alpizar, S. Guilloteau +22

Context: Investigating the vertical distribution of molecular content in protoplanetary disks remains difficult in most disks mildly inclined along the line of sight. In contrast,…

astro-ph.EP2025★ 4 cited

Edge-On Disk Study (EODS) II: Thermal Structure of the Flying Saucer Disk

S. Guilloteau, O. Denis-Alpizar, A. Dutrey +21

Context. The dust and gas temperature in proto-planetary disks play critical roles in determining their chemical evolution and influencing planet formation processes. Aims. We atte…

astro-ph.EP2025★ 1 cited

Impact of rotation on synthetic mass-radius relationships of two-layer rocky planets and water worlds

J. -M. Huré, P. Noé, C. Staelen +1

We have analyzed the effects of rotation on mass-radius relationships for single-layer and two-layer planets having a core and an envelope made of pure materials among iron, perovs…

astro-ph.EP2024

Existence of slowly rotating bipolytropes with prolate cores

Clément Staelen, Jean-Marc Huré, Anaïs Meunier +1

We report the existence of hydrostatic equilibrium states for a composite body made of two rigidly rotating, homogeneous layers bounded by spheroidal surfaces, where the core has a…

astro-ph.GA2024

The Maclaurin spheroid in disguise. New figures of equilibrium with external magnetic support

Jean-Marc Huré, Clément Staelen

We show that a rigidly rotating, homogeneous ellipsoid of revolution threaded by a uniform, coaxial magnetic field is a possible figure of equilibrium. While the spheroidal shape i…

astro-ph.SR2024

Approaching the structure of rotating bodies from dimension reduction

Clément Staelen, Jean-Marc Huré

We show that the two-dimensional structure of a rigidly rotating self-gravitating body is accessible with relatively good precision by assuming a purely spheroidal stratification.…