activity
20152019
most citedOn the consistent treatment of the quasi-hydrostatic layers in hot star atmospheres

154 citations · 489 across the 8 of their papers we have counts for

collaborators

14 papers

astro-ph.SR202039 cited

The stellar and wind parameters of six prototypical HMXBs and their evolutionary status

R. Hainich, L. M. Oskinova, J. M. Torrejón +7

High-mass X-ray binaries (HMXBs) are exceptional astrophysical laboratories that offer a rare glimpse into the physical processes that govern accretion on compact objects, massive-…

astro-ph.SR2019

The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud: spectroscopy, orbital analysis, formation, and evolution

T. Shenar, D. P. Sablowski, R. Hainich +11

Massive Wolf-Rayet (WR) stars dominate the radiative and mechanical energy budget of galaxies and probe a critical phase in the evolution of massive stars prior to core-collapse. I…

astro-ph.SR2019117 cited

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

Varsha Ramachandran, W. -R. Hamann, L. M. Oskinova +6

Stars which start their lives with spectral types O and early-B are the progenitors of core-collapse supernovae, long gamma-ray bursts, neutron stars, and black holes. These massiv…

astro-ph.SR2019121 cited

The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters

W. -R. Hamann, G. Gräfener, A. Liermann +6

Comprehensive spectral analyses of the Galactic Wolf-Rayet stars of the nitrogen sequence (i.e.\ the WN subclass) have been performed in a previous paper. However, the distances of…

astro-ph.HE2018

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.SR2018

PoWR grids of non-LTE model atmospheres for OB-type stars of various metallicities

R. Hainich, V. Ramachandran, T. Shenar +5

The study of massive stars in different metallicity environments is a central topic of current stellar research. The spectral analysis of massive stars requires adequate model atmo…