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20162022
most citedForming spectroscopic massive proto-binaries by disk fragmentation

97 citations · 370 across the 13 of their papers we have counts for

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12 papers · 1 filter

astro-ph.SR202216 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.SR202210 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.SR202117 cited

On the bipolarity of Wolf-Rayet nebulae

D. M. -A. Meyer

Wolf-Rayet stars are amongst the rarest but also most intriguing massive stars. Their extreme stellar winds induce famous multi-wavelength circumstellar gas nebulae of various morp…

astro-ph.SR202130 cited

3D MHD astrospheres: applications to IRC-10414 and Betelgeuse

D. M. -A. Meyer, A. Mignone, M. Petrov +3

A significative fraction of all massive stars in the Milky Way move supersonically through their local interstellar medium (ISM), producing bow shock nebulae by wind-ISM interactio…

astro-ph.SR202031 cited

Parameter study for the burst mode of accretion in massive star formation

D. M. -A. Meyer, E. I. Vorobyov, V. G. Elbakyan +3

It is now a widely held view that, in their formation and early evolution, stars build up mass in bursts. The burst mode of star formation scenario proposes that the stars grow in…

astro-ph.SR202018 cited

On the ring nebulae around runaway Wolf-Rayet stars

D. M. -A. Meyer, L. M. Oskinova, M. Pohl +1

Wolf-Rayet stars are advanced evolutionary stages of massive stars. Despite their large mass-loss rates and high wind velocities, none of them display a bow shock, although a fract…