activity
20102026
most citedStellar feedback efficiencies: supernovae versus stellar winds

96 citations · 353 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

The birth and fate of stellar clumps in super-early galaxies

B. Das, A. Ferrara, A. Pallottini +2

(Abridged) JWST has revealed extremely compact stellar clumps in galaxies at z>6, but their formation mechanism and subsequent evolution remain uncertain. We investigate whether su…

astro-ph.GA2026

On the clumpy nature of super-early galaxies

A. Ferrara, B. Das, M. Kohandel +2

JWST has revealed that galaxies during the Epoch of Reionization are composed of compact stellar clumps spanning more than two orders of magnitude in mass and size. We present an a…

astro-ph.GA2021★ 28 cited

Strong dependence of the physical properties of cores on spatial resolution in observations and simulations

Fabien Louvet, Patrick Hennebelle, Alexander Men'shchikov +3

During the last decade in star formation research, many studies have targeted low- and high-mass star formation regions located at different distances, with different telescopes ha…

astro-ph.GA2019★ 32 cited

The core and stellar mass functions in massive collapsing filaments

Evangelia Ntormousi, Patrick Hennebelle

The connection between the pre-stellar core mass function (CMF) and the stellar initial mass function (IMF) lies at the heart of all star formation theories. In this paper, we stud…

astro-ph.GA2017★ 46 cited

The role of magnetic fields in the structure and interaction of supershells

Evangelia Ntormousi, Joanne R. Dawson, Patrick Hennebelle +1

Large-scale shocks formed by clustered feedback of young OB stars are considered an important source of mechanical energy for the ISM and a trigger of molecular cloud formation. Th…

astro-ph.GA2016★ 38 cited

The effect of ambipolar diffusion on low-density molecular ISM filaments

Evangelia Ntormousi, Patrick Hennebelle, Philippe André +1

The filamentary structure of the molecular interstellar medium and the potential link of this morphology to star formation have been brought into focus recently by high resolution…