most citedA synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models

39 citations · 126 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.SR202239 cited

A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models

D. Pauli, N. Langer, D. R. Aguilera-Dena +2

Without doubt, mass transfer in close binary systems contributes to the populations of Wolf-Rayet (WR) stars in the Milky Way and the Magellanic Clouds. However, the binary formati…

astro-ph.HE202222 cited

Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution

V. Ramachandran, L. M. Oskinova, W. -R. Hamann +10

M33 X-7 is the only known eclipsing black hole high mass X-ray binary. The system is reported to contain a very massive O supergiant donor and a massive black hole in a short orbit…

astro-ph.SR202236 cited

Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC346 in the SMC galaxy

M. J. Rickard, R. Hainich, W. -R. Hamann +9

Massive stars are among the main cosmic engines driving the evolution of star-forming galaxies. Their powerful ionising radiation and stellar winds inject a large amount of energy…

astro-ph.SR202129 cited

Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations

David R. Aguilera-Dena, Norbert Langer, John Antoniadis +5

Massive stars that become stripped of their hydrogen envelope through binary interaction or winds can be observed either as Wolf-Rayet stars, if they have optically thick winds, or…