activity
20092026
most citedHST/STIS Ultraviolet Spectroscopy of the Components of the Massive Triple Star delta Ori A

197 citations · 808 across the 30 of their papers we have counts for

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27 papers · 1 filter

astro-ph.SR2026

Unresolved triple systems in the aged open cluster Trumpler 19: Discovery, confirmation, and implications

D. Minniti, R. K. Saito, V. D. Ivanov +31

It is difficult to identify unresolved triple and higher-order systems beyond the solar vicinity. Star clusters yield controlled environments with known physical parameters, provid…

astro-ph.SR2021★ 33 cited

Analysis of physical processes in eruptive YSOs with near infrared spectra and multi-wavelength light curves

Zhen Guo, P. W. Lucas, C. Contreras Peña +11

The decade-long Vista Variables in the Via Lactea (VVV) survey has detected numerous highly variable young stellar objects (YSOs). We present a study of 61 highly variable VVV YSOs…

astro-ph.SR2021★ 8 cited

Conditions in the WR 140 wind-collision region revealed by the 1.083-micron He I line profile

Peredur M. Williams, Watson P. Varricatt, André-Nicolas Chené +10

We present spectroscopy of the P~Cygni profile of the 1.083-micron He I line in the WC7 + O5 colliding-wind binary (CWB) WR 140 (HD 193793), observed in 2008, before its periastron…

astro-ph.SR2020★ 17 cited

Clumping in the Winds of Wolf-Rayet Stars

André-Nicolas Chené, Nicole St-Louis, Anthony F. J. Moffat +1

We attempt to determine the driver for clumping in hot-star winds by extending the measure of the spectral variability level of Galactic Wolf-Rayet stars to by far the hottest know…

astro-ph.SR2019★ 6 cited

Massive stars in the young cluster VVV CL074

F. Martins, A. N. Chené, J. -C. Bouret +4

We obtained K-band spectroscopy of the brightest members of the cluster VVV CL074 in order to identify the massive star population. We also determined the stellar properties of the…

astro-ph.SR2019★ 14 cited

Investigating the origin of the spectral line profiles of the Hot Wolf-Rayet Star WR2

A. -N. Chené, N. St-Louis, A. F. J. Moffat +12

The hot WN star WR2 (HD6327) has been claimed to have many singular characteristics. To explain its unusually rounded and relatively weak emission line profiles, it has been propos…