9 citations · 9 across the 3 of their papers we have counts for
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astro-ph.SR2026
The upper main sequence in h and chi Persei
A. Marco, I. Negueruela, N. Castro +1
Binary interactions play a crucial role in the evolution and eventual outcomes of massive stars. Rich young open clusters provide large coeval populations to constrain the effects…
astro-ph.SR2026
Astrophysical parameters of LS 437 and the nature of X0726-260
Ignacio Negueruela, Sara R. Berlanas, Lee J. Townsend +2
Be/X-ray binaries, the most common class of high-mass X-ray binaries, are characterised by OBe companions, but display a rich variety of X-ray behaviours. One of the most atypical…
astro-ph.SR2023★ 9 cited
To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars
K. Rübke, A. Herrero, J. Puls
Winds of massive stars have density inhomogeneities (clumping) that may affect the formation of spectral lines in different ways, depending on their formation region. Most of previ…