activity
20012016
most citedThe PLATO 2.0 Mission

1.3k citations · 2.2k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.SR2016★ 49 cited

Bow shock nebulae of hot massive stars in a magnetized medium

D. M. -A. Meyer, A. Mignone, R. Kuiper +2

A significant fraction of OB-type, main-sequence massive stars are classified as runaway and move supersonically through the interstellar medium (ISM). Their strong stellar winds i…

astro-ph.SR2016★ 146 cited

On the existence of accretion-driven bursts in massive star formation

D. M. -A. Meyer, E. I. Vorobyov, R. Kuiper +1

Accretion-driven luminosity outbursts are a vivid manifestation of variable mass accretion onto protostars. They are known as the so-called FU Orionis phenomenon in the context of…

astro-ph.SR2016★ 40 cited

On the observability of bow shocks of Galactic runaway OB stars

D. M. -A. Meyer, A. -J. van Marle, R. Kuiper +1

Massive stars that have been ejected from their parent cluster and supersonically sailing away through the interstellar medium (ISM) are classified as exiled. They generate circums…

astro-ph.EP2013★ 1.3k cited

The PLATO 2.0 Mission

H. Rauer, C. Catala, C. Aerts +159

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it…

astro-ph.SR2011★ 24 cited

Global Structure of Magnetorotationally Turbulent Protoplanetary Discs

M. Flaig, P. Ruoff, W. Kley +1

The aim of the present paper is to investigate the spatial structure of a protoplanetary disc whose dynamics is governed by magnetorotational turbulence. We perform a series of loc…

astro-ph.EP2011★ 37 cited

Collisions of inhomogeneous pre-planetesimals

R. J. Geretshauser, R. Speith, W. Kley

In the framework of the coagulation scenario, kilometre-sized planetesimals form by subsequent collisions of pre-planetesimals of sizes from centimetre to hundreds of metres. Pre-p…