activity
20162021
most citedAnalytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure

62 citations · 243 across the 8 of their papers we have counts for

collaborators

14 papers

astro-ph.SR202120 cited

Shock-heated radiation-driven outflows as a solution to the weak-wind problem of late O-type stars

C. Lagae, F. A. Driessen, L. Hennicker +2

Context. Radiation-driven mass loss is key to our understanding of massive-star evolution. However, for low-luminosity O-type stars there are big discrepancies between theoreticall…

astro-ph.SR202162 cited

Analytic, dust-independent mass-loss rates for red supergiant winds initiated by turbulent pressure

N. D. Kee, J. O. Sundqvist, L. Decin +2

Context. Red supergiants are observed to undergo vigorous mass-loss. However, to date, no theoretical model has succeeded in explaining the origins of these objects' winds. This st…

astro-ph.SR202031 cited

Dynamically inflated wind models of classical Wolf-Rayet stars

L. G. Poniatowski, J. O. Sundqvist, N. D. Kee +6

Vigorous mass loss in the classical Wolf-Rayet (WR) phase is important for the late evolution and final fate of massive stars. We develop spherically symmetric time-dependent and s…

astro-ph.SR2020

Line-drag damping of Alfvén waves in radiatively driven winds of magnetic massive stars

F. A. Driessen, N. D. Kee, J. O. Sundqvist +1

Line-driven stellar winds from massive (OB) stars are subject to a strong line-deshadowing instability. Recently, spectropolarimetric surveys have collected ample evidence that a s…

astro-ph.SR202021 cited

A Detailed View of the Circumstellar Environment and Disk of the Forming O-star AFGL 4176

K. G. Johnston, M. G. Hoare, H. Beuther +5

We present a detailed analysis of the disk and circumstellar environment of the forming O-type star AFGL 4176 mm1, placing results from the Atacama Large Millimeter/submillimeter A…

astro-ph.SR201953 cited

Spiral arms and instability within the AFGL 4176 mm1 disc

K. G. Johnston, M. G. Hoare, H. Beuther +7

We present high-resolution (30 mas or 130 au at 4.2 kpc) Atacama Large Millimeter/submillimeter Array observations at 1.2 mm of the disc around the forming O-type star AFGL 4176 mm…