activity
20182021
most citedConstraining mixing in massive stars in the Small Magellanic Cloud

130 citations · 246 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2021

Modeling non-thermal emission from SN 1987A

Robert Brose, Jonathan Mackey, Sean Kelly +2

The remnant of SN 1987A is the best-studied object of its kind. The rich data-set of its thermal and non-thermal emission across the electromagnetic spectrum poses a unique testbed…

astro-ph.SR201967 cited

The Tarantula Massive Binary Monitoring: III. Atmosphere analysis of double-lined spectroscopic systems

L. Mahy, H. Sana, M. Abdul-Masih +17

Accurate stellar parameters of individual objects in binary systems are essential to constrain the effects of binarity on stellar evolution. These parameters serve as a prerequisit…

astro-ph.SR201949 cited

The Tarantula Massive Binary Monitoring. IV. Double-lined photometric binaries

L. Mahy, L. A. Almeida, H. Sana +10

A high fraction of massive stars are found to be binaries but only a few of them are reported as photometrically variable. By studying the populations of SB2 in the 30 Doradus regi…

astro-ph.SR2019

Properties of OB star-black hole systems derived from detailed binary evolution models

N. Langer, C. Schürmann, K. Stoll +38

The recent gravitational wave measurements have demonstrated the existence of stellar mass black hole binaries. It is essential for our understanding of massive star evolution to i…

astro-ph.SR2019130 cited

Constraining mixing in massive stars in the Small Magellanic Cloud

Abel Schootemeijer, Norbert Langer, Nathan J. Grin +1

Context. The evolution of massive stars is strongly influenced by internal mixing processes such as semiconvection, convective core overshooting, and rotationally induced mixing. N…

astro-ph.SR2018

Subsonic structure and optically thick winds from Wolf--Rayet stars

Luca Grassitelli, Norbert Langer, Nathan J. Grin +3

Wolf-Rayet star's winds can be so dense and so optically thick that the photosphere appears in the highly supersonic part of the outflow, veiling the underlying subsonic part of th…