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Wolf-Rayet stars in the Small Magellanic Cloud: I. Analysis of the single WN stars
R. Hainich, D. Pasemann, H. Todt +3
Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ionizing radiation fields and powerful stellar winds. Since these winds are considered to be…
The donor star of the X-ray pulsar X1908+075
Silvia Martínez-Núñez, Andreas Sander, Ángel Gímenez-García +4
High-mass X-ray binaries (HMXBs) consist of a massive donor star and a compact object. While several of those systems have been well studied in X-rays, little is known for most of…
On the consistent treatment of the quasi-hydrostatic layers in hot star atmospheres
Andreas Sander, Tomer Shenar, Rainer Hainich +3
CONTEXT: Spectroscopic analysis remains the most common method to derive masses of massive stars, the most fundamental stellar parameter. While binary orbits and stellar pulsations…