activity
20152022
most citedThe accretion rates and mechanisms of Herbig Ae/Be stars

112 citations · 195 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2022★ 8 cited

Tracing a decade of activity towards a yellow hypergiant. The spectral and spatial morphology of IRC+10420 at au scales

Evgenia Koumpia, R. D. Oudmaijer, W. -J. de Wit +3

The fate of a massive star during the latest stages of its evolution is highly dependent on its mass-loss history and geometry, with the yellow hypergiants being key objects to stu…

astro-ph.SR2020★ 112 cited

The accretion rates and mechanisms of Herbig Ae/Be stars

C. Wichittanakom, R. D. Oudmaijer, J. R. Fairlamb +3

This work presents a spectroscopic study of 163 Herbig Ae/Be stars. Amongst these, we present new data for 30 objects. Stellar parameters such as temperature, reddening, mass, lumi…

astro-ph.SR2019★ 10 cited

Resolving the MYSO binaries PDS 27 and PDS 37 with VLTI/PIONIER

E. Koumpia, K. M. Ababakr, W. J. de Wit +7

Binarity and multiplicity appear to be a common outcome in star formation. In particular, the binary fraction of massive (OB-type) stars can be very high. In many cases, the furthe…

astro-ph.SR2017★ 42 cited

A Statistical Spectropolarimetric Study of Herbig Ae/Be Stars

Karim Ababakr, Rene Oudmaijer, Jorick Vink

We present Halpha linear spectropolarimetry of a large sample of Herbig Ae/Be stars. Together with newly obtained data for 17 objects, the sample contains 56 objects, the largest s…

astro-ph.SR2016★ 11 cited

Linear spectropolarimetry across the optical spectrum of Herbig Ae/Be stars

K. M. Ababakr, R. D. Oudmaijer, J. S. Vink

We present the results of spectropolarimetric observations of 12 Herbig Ae/Be objects. Our data have the largest spectropolarimetric wavelength coverage, 4560 Å to 9480 Å, publishe…

astro-ph.SR2015★ 12 cited

Spectroscopy and Linear Spectropolarimetry of the early Herbig Be Stars PDS 27 and PDS 37

K. M. Ababakr, J. R. Fairlamb, R. D. Oudmaijer +1

The number of well-studied early-type pre-main-sequence objects is very limited, hampering the study of massive star formation from an observational point of view. Here, we present…