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20222026
most citedX-Shooting ULLYSES: massive stars at low metallicity. I. Project Description

61 citations · 302 across the 32 of their papers we have counts for

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astro-ph.IM2026

The critical role of HST UV spectroscopy in constraining red supergiant binary systems

Daniel Jadlovský, Andreas Sander, Lee Patrick +3

The Hubble Space Telescope (HST) has advanced our knowledge of stellar evolution thanks to its unique high-spectral resolution and high-sensitivity capabilities in the UV region, e…

astro-ph.SR2026★ 1 cited

X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates

O. Verhamme, J. O. Sundqvist, A. de Koter +21

Context. For stellar evolution models we rely on mass-loss rate prescriptions that show features that lack empirical confirmation, such as the bi-stability jump. This jump is an in…

astro-ph.SR2026

The winds of OBA hypergiants and luminous blue variables: Dynamically-consistent atmosphere models reveal multiple wind regimes

Matheus Bernini-Peron, Andreas A. C. Sander, Gautham N. Sabhahit +3

OBA hypergiants (OBAHGs) are evolved massive stars with notable wind features in their optical spectrum. Located at the cool edge of the line-driven wind regime, many are candidate…

astro-ph.SR2026★ 1 cited

X-Shooting ULLYSES: Massive stars at low metallicity XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds

T. Alkousa, P. A. Crowther, J. M. Bestenlehner +10

Considering the physics of radiation-driven winds of massive stars, the wind properties should depend on the metal content of the stellar atmosphere. Therefore, studying the winds…

astro-ph.SR2026★ 2 cited

Dynamically consistent analysis of Galactic WN4b stars

Roel R. Lefever, Andreas A. C. Sander, Matheus Bernini-Peron +6

Many Wolf-Rayet (WR) stars have optically thick winds that cloak the hydrostatic layers of the underlying star. In these cases, traditional spectral analysis methods are plagued by…