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19992026
most citedMass-loss predictions for O and B stars as a function of metallicity

1.7k citations · 12.3k across the 196 of their papers we have counts for

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Showing 2005 · astro-phShow all

7 papers · 2 filters

astro-ph2005★ 6 cited

Massive star feedback - from the first stars to the present

Jorick S. Vink

The amount of mass loss is of fundamental importance to the lives and deaths of very massive stars, the input of chemical elements and momentum into the interstellar and intergalac…

astro-ph2005

The clumpiness of Luminous Blue Variable winds

Ben Davies, Rene D. Oudmaijer, Jorick S. Vink

We present the first systematic spectropolarimetric study of Luminous Blue Variables (LBVs), and find that at least half those objects studied display evidence for intrinsic polari…

astro-ph2005★ 14 cited

Near-infrared line spectropolarimetry of hot massive stars

R. D. Oudmaijer, J. E. Drew, J. S. Vink

In order to study the inner parts of the circumstellar material around optically faint, infrared bright objects, we present the first medium-resolution spectropolarimetric data tak…

astro-ph2005★ 466 cited

On the metallicity dependence of Wolf-Rayet winds

Jorick S. Vink, Alex de Koter

We have performed a pilot study of mass loss predictions for late-type Wolf-Rayet (WR) stars as a function of metal abundance, over a range between 10^{-5} < (Z/Zsun) < 10. We find…

astro-ph2005★ 1 cited

The INT Photometric H-alpha Survey of the Northern Galactic Plane (IPHAS)

Janet E. Drew, R. Greimel, M. J. Irwin +1

The INT Photometric Halpha Survey of the Northern Galactic Plane (IPHAS) is a 1800 square degrees CCD survey of the northern Milky Way spanning the latitude range -5 < b < +5 (degr…

astro-ph2005★ 20 cited

On the origin of the X-ray emission towards the early Herbig Be star MWC 297

Jorick S. Vink, Paul M. O'Neill, Sebastian G. Els +1

We present high resolution AO-corrected coronographic near-infrared imaging on the early-type Herbig Be star MWC 297. X-ray flaring has been reported towards this young object, how…