activity
20032026
most citedEarly magnetic B-type stars: X-ray emission and wind properties

118 citations · 1k across the 30 of their papers we have counts for

collaborators

30 papers

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…

astro-ph.SR2025

Discovery of a new transitional type of evolved massive stars with hard ionizing flux

Andreas A. C. Sander, Roel R. Lefever, Joris Josiek +12

Wolf-Rayet (WR) stars are the evolved descendants of the most massive stars and show emission-line dominated spectra formed in their powerful stellar winds. Marking the final evolu…

astro-ph.GA2019★ 5 cited

Testing massive star evolution, star-formation history, and feedback at low metallicity: Photometric analysis of OB stars in the SMC Wing

Leah M. Fulmer, John S. Gallagher, Wolf-Rainer Hamann +2

The supergiant ionized shell SMC-SGS 1 (DEM 167), located in the outer Wing of the Small Magellanic Cloud (SMC), resembles structures that originate from an energetic star-formatio…

astro-ph.HE2018★ 17 cited

On the apparent absence of WR+NS systems: the curious case of WR124

J. A. Toala, L. M. Oskinova, W. -R. Hamann +8

Among different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf-Rayet (WR) stars with this spectral type in our Galaxy.…

astro-ph.GA2018★ 66 cited

Stellar population of the superbubble N206 in the LMC II. Parameters of the OB and WR stars, and the total massive star feedback

Varsha Ramachandran, W. -R. Hamann, R. Hainich +5

Clusters or associations of early-type stars are often associated with a 'superbubble' of hot gas. The formation of such superbubbles is caused by the feedback from massive stars.…

astro-ph.SR2016★ 22 cited

The Tarantula Massive Binary Monitoring project: II. A first SB2 orbital and spectroscopic analysis for the Wolf-Rayet binary R145

T. Shenar, N. D. Richardson, D. P. Sablowski +19

We present the first SB2 orbital solution and disentanglement of the massive Wolf-Rayet binary R145 (P = 159d) located in the Large Magellanic Cloud. The primary was claimed to hav…