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20022008
most citedProperties of WNh stars in the Small Magellanic Cloud: evidence for homogeneous evolution

71 citations · 152 across the 5 of their papers we have counts for

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astro-ph2005

Dust Production in the High-Redshift Universe

S. V. Marchenko

How much dust can be produced in the early Universe? Does dust production depend on the average heavy-metal content of the hosting galaxy? Considering supernova explosions, massive…

astro-ph2005

Wind ionization structure of the short-period eclipsing LMC Wolf-Rayet binary BAT99-129: preliminary results

C. Foellmi, A. F. J. Moffat, S. V. Marchenko

BAT99-129 is a rare, short-period eclipsing Wolf-Rayet binary in the Large Magellanic Cloud. We present here medium-resolution NTT/EMMI spectra that allow us to disentangle the spe…

astro-ph2005

The Wolf-Rayet hydrogen puzzle -- an observational point of view

C. Foellmi, S. V. Marchenko, A. F. J. Moffat

Significant amounts of hydrogen were found in very hot early-type single WN stars in the SMC and the LMC. Recently, we found similar evidence in the Wolf-Rayet star of a short-peri…

astro-ph2005

The massive eclipsing LMC Wolf-Rayet binary BAT99-129. 1 Orbital parameters, hydrogen content and spectroscopic characteristics

C. Foellmi, A. F. J. Moffat, S. V. Marchenko

BAT99-129 in the LMC is one among a handful of extra-galactic eclipsing Wolf-Rayet binaries known. We present blue, medium-resolution, phase-dependent NTT-EMMI spectra of this syst…

astro-ph2005

Stellar Model Analysis of the Oscillation Spectrum of eta Bootis Obtained from MOST

D. B. Guenther, T. Kallinger, P. Reegen +8

Eight consecutive low-frequency radial p-modes are identified in the G0 IV star eta Bootis based on 27 days of ultraprecise rapid photometry obtained by the MOST (Microvariability…

astro-ph2005

Spectroscopic study of the long-period dust-producing WC7pd+O9 binary HD192641

L. Lefevre, S. V. Marchenko, S. Lepine +12

We present the results of an optical spectroscopic study of the massive Wolf-Rayet binary WR137. These data cover the dust-formation maximum in 1997. Combining all available measur…