activity
20122024
most citedOn the existence of accretion-driven bursts in massive star formation

146 citations · 1.1k across the 43 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.SR2022★ 16 cited

Episodic accretion and mergers during growth of massive protostars

Vardan G. Elbakyan, Sergei Nayakshin, Dominique M. -A. Meyer +1

3D simulations of high mass young stellar object (HMYSO) growth show that their circumstellar discs fragment onto multiple self-gravitating objects. Accretion of these by HMYSO may…

astro-ph.SR2022★ 10 cited

The burst mode of accretion in massive star formation with stellar inertia

D. M. -A. Meyer, E. I. Vorobyov, V. G. Elbakyan +4

The burst mode of accretion in massive star formation is a scenario linking the initial gravitational collapse of parent pre-stellar cores to the properties of their gravitationall…

astro-ph.SR2022★ 2 cited

Discovery of an optical cocoon tail behind the runaway HD 185806

Z. T. Spetsieri, P. Boumis, A. Chiotellis +6

Studies on the circumstellar structures around evolved stars provide vital information on the evolution of the parent star and the properties of the local interstellar medium. In t…

astro-ph.HE2022★ 17 cited

Rectangular core-collapse supernova remnants: application to Puppis A

D. M. -A. Meyer, P. F. Velazquez, O. Petruk +9

Core-collapse supernova remnants are the gaseous nebulae of galactic interstellar media (ISM) formed after the explosive death of massive stars. Their morphology and emission prope…

astro-ph.HE2022★ 11 cited

Pulsar wind nebulae of runaway massive stars

D. M. -A. Meyer, Z. Meliani

A significant fraction of massive stars move at speed through the interstellar medium of galaxies. After their death as core collapse supernovae, a possible final evolutionary stat…

astro-ph.HE2022★ 23 cited

Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble

Samata Das, Robert Brose, Dominique M. -A. Meyer +3

Context. Galactic cosmic rays are widely assumed to arise from diffusive shock acceleration, specifically at shocks in supernova remnants (SNRs). These shocks expand in a complex e…