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Stellar models with rotation. 0.8<M<120, Z=0.014
Many topical astrophysical research areas, such as the properties of planet host stars, the nature of the progenitors of different types of supernovae and gamma ray bursts, and... -
Galactic massive stars with AstraLux
Massive stars have high-multiplicity fractions, and many of them have still undetected components, thus hampering the study of their properties. I study a sample of massive... -
Dust formation in WC stars
The following table gives the ratefile of the chemical model. Columns {alpha}, {beta} and {gamma} give the rate k at temperature T in the Arrhenius form: k = {alpha} *... -
Planetary nebulae with WR-type nuclei
A recent systematic search of Wolf-Rayet features in the spectra of Galactic planetary nebulae has increased the list of objects that are known to have WR-type nuclei to about... -
Radio emission from stars at 250GHz
We have used the IRAM 30 m-telescope together with the Max Planck Institute for Radio Astronomy (MPIfR) bolometer to survey nearly 270 stars of different types for 250GHz... -
RXTE, Swift & NICER obs. of WR 140
The long-period, highly eccentric Wolf-Rayet star binary system WR140 has exceptionally well-determined orbital and stellar parameters. Bright, variable X-ray emission is... -
Wolf-Rayet stars in Large Magellanic Cloud
Massive stars, although being important building blocks of galaxies, are still not fully understood. This especially holds true for Wolf-Rayet (WR) stars with their strong mass... -
Annex to 7th Cat. of Galactic WR Stars
This paper gathers, from the literature and private communication, 72 new Galactic Population I Wolf-Rayet stars and 17 candidate WCLd stars, recognized and/or discovered after... -
7th Catalog of Galactic Wolf-Rayet stars
The VIIth catalogue of galactic Population I Wolf Rayet stars provides improved coordinates, spectral types and bv photometry of known WR stars and adds 71 new WR stars to the...