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20032014
most citedThe Wolf-Rayet stars in the Large Magellanic Cloud: A comprehensive analysis of the WN class

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

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30 papers

astro-ph.SR2014★ 204 cited

The Wolf-Rayet stars in the Large Magellanic Cloud: A comprehensive analysis of the WN class

R. Hainich, U. Rühling, H. Todt +6

Aims: Following our comprehensive studies of the WR stars in the Milky Way, we now present spectroscopic analyses of almost all known WN stars in the LMC. Methods: For the quantita…

astro-ph.SR2011★ 13 cited

A 10-hour period revealed in optical spectra of the highly variable WN8 Wolf-Rayet star WR 123

A. -N. Chené, C. Foellmi, S. V. Marchenko +6

Aims. What is the origin of the large-amplitude variability in Wolf-Rayet WN8 stars in general and WR123 in particular? A dedicated spectroscopic campaign targets the ten-hour peri…

astro-ph.SR2010★ 20 cited

A brown dwarf companion to the intermediate-mass star HR6037

N. Huelamo, D. E. A. Nuernberger, V. D. Ivanov +8

In the course of an imaging survey we have detected a visual companion to the intermediate-mass star HR 6037. In this letter, we present two epoch observations of the binary with N…

astro-ph.HE2010★ 31 cited

The pertinence of Jet Emitting Discs physics to Microquasars: Application to Cygnus X-1

P. O. Petrucci, J. Ferreira, G. Henri +2

The interpretation of the X-ray spectra of X-ray binaries during their hard states requires a hot, optically thin medium. There are several accretion disc models in the literature…

astro-ph2008★ 18 cited

What is the closest black hole to the Sun?

C. Foellmi

We examine the distance of the two galactic microquasars GRO J1655-40 and A0620-00, which are potentially the two closest black holes to the Sun. We aim to provide a picture as wid…

astro-ph2008★ 71 cited

Properties of WNh stars in the Small Magellanic Cloud: evidence for homogeneous evolution

F. Martins, D. J. Hillier, J. C. Bouret +4

We derive the physical properties of three WNh stars in the SMC to constrain stellar evolution beyond the main sequence at low metallicity and to investigate the metallicity depend…