activity
20172026
most citedThe first interferometric survey in the K-band of massive YSOs. On the hot dust, ionised gas, and binarity at au scales

18 citations · 38 across the 10 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR2026

Ionized gas emission in protoplanetary disks with the SKAO

Greta Guidi, Christian Rab, Barbara Ercolano +20

Protoplanetary disks represent a crucial stage in the evolution of Young Stellar Objects towards the formation of fully formed planetary systems. While substantial progress has bee…

astro-ph.SR2026

Spatial and spectral constraints on resolved mass-loss of the massive Post-RSG star IRAS 17163-3907 and its Fried Egg Nebula

E. Koumpia, A. Cikota, W. -J. de Wit +12

The fate of massive stars during the latest stages of their evolution is highly dependent on their mass-loss rate and geometry. These processes have a significant influence on star…

astro-ph.SR2023

The RMS survey: a census of massive YSO multiplicity in the -band

Robert G. Shenton, Rebecca J. Houghton, René D. Oudmaijer +4

Close to 100 per cent of massive stars are thought to be in binary systems. The multiplicity of massive stars seems to be intrinsically linked to their formation and evolution, and…

astro-ph.SR20221 cited

First spatially resolved Na I and He I transitions towards an MYSO. Finding new tracers for the gaseous star/disc interface

Evgenia Koumpia, M. Koutoulaki, W. -J. de Wit +4

With steady observational advances, the formation of massive stars is being understood in more detail. Numerical models are converging on a scenario where accretion discs play a ke…

astro-ph.SR202118 cited

The first interferometric survey in the K-band of massive YSOs. On the hot dust, ionised gas, and binarity at au scales

E. Koumpia, W. -J. de Wit, R. D. Oudmaijer +8

Circumstellar discs are essential for high mass star formation, while multiplicity, in particular binarity, appears to be an inevitable outcome since the vast majority of massive s…

astro-ph.SR20219 cited

K-band GRAVITY/VLTI interferometry of "extreme" Herbig Be stars. The size-luminosity relation revisited

P. Marcos-Arenal, I. Mendigutía, E. Koumpia +7

(Abridged:) It has been hypothesized that the location of Herbig Ae/Be stars (HAeBes) within the empirical relation between the inner disk radius (r), inferred from K-band i…