activity
19942009
most citedThe empirical metallicity dependence of the mass-loss rate of O- and early B-type stars

317 citations · 2.2k across the 19 of their papers we have counts for

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Showing 2005Show all

9 papers · 1 filter

astro-ph2005

The 10 micron amorphous silicate feature of fractal aggregates and compact particles with complex shapes

M. Min, C. Dominik, J. W. Hovenier +2

We model the 10 micron absorption spectra of nonspherical particles composed of amorphous silicate. We consider two classes of particles, compact ones and fractal aggregates compos…

astro-ph2005

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

Spectral analysis of early-type stars using a genetic algorithm based fitting method

M. R. Mokiem, A. de Koter, J. Puls +3

We present the first automated fitting method for the quantitative spectroscopy of O- and early B-type stars with stellar winds. The method combines the non-LTE stellar atmosphere…

astro-ph2005

The composition and size distribution of the dust in the coma of comet Hale-Bopp

M. Min, J. W. Hovenier, A. de Koter +2

We discuss the composition and size distribution of the dust in the coma of comet Hale-Bopp. We do this by fitting simultaneously the infrared emission spectrum measured by the inf…

astro-ph2005

The VLT-FLAMES Survey of Massive Stars: Observations in the Galactic Clusters NGC 3293, NGC 4755 and NGC 6611

C. J. Evans, S. J. Smartt, J. -K. Lee +23

We introduce a new survey of massive stars in the Galaxy and the Magellanic Clouds using the Fibre Large Array Multi-Element Spectrograph (FLAMES) instrument at the Very Large Tele…

astro-ph2005

A 10 micron spectroscopic survey of Herbig Ae star disks: grain growth and crystallization

R. van Boekel, M. Min, L. B. F. M. Waters +4

We present spectroscopic observations of a large sample of Herbig Ae stars in the 10 micrometer spectral region. We perform compositional fits of the spectra based on properties of…