activity
20162020
most citedThe Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system

32 citations · 80 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020★ 1 cited

The photometric and polarimetric variability of magnetic O-type stars

Melissa Munoz, Gregg Wade, Daniel Faes +1

Massive star winds are important contributors to the energy, momentum and chemical enrichment of the interstellar medium. Strong, organized and predominantly dipolar magnetic field…

astro-ph.SR2020★ 2 cited

MOBSTER: Identifying Candidate Magnetic O Stars through Rotational Modulation of TESS Photometry

James Barron, Gregg A. Wade, Dominic M. Bowman +4

Being relatively rare, the properties of magnetic O stars are not fully understood. To date fewer than a dozen of these stars have been confirmed, making any inference of their glo…

astro-ph.SR2019★ 13 cited

Modelling the photometric variability of magnetic massive stars with the Analytical Dynamical Magnetosphere model

M. S. Munoz, G. A. Wade, Y. Nazé +3

In this paper, we investigate the photometric variability of magnetic O-type stars. Such stars possess oblique, predominantly dipolar magnetic fields that confine their winds rough…

astro-ph.SR2018★ 32 cited

The Shortest-period Wolf-Rayet binary in the Small Magellanic Cloud: Part of a high-order multiple system

T. Shenar, R. Hainich, H. Todt +8

SMC AB 6 is the shortest-period (6.5d) Wolf-Rayet (WR) binary in the Small Magellanic Cloud, and is therefore crucial for the study of binary interaction and formation of WR stars…

astro-ph.SR2018★ 1 cited

The Of?p stars of the Magellanic Clouds: Are they strongly magnetic?

Melissa Munoz, Gregg Wade, Yaël Nazé +2

All known Galactic Of?p stars have been shown to host strong, organized, magnetic fields. Recently, five Of?p stars have been discovered in the Magellanic Clouds. They posses photo…

astro-ph.SR2016★ 11 cited

WR 148: Identifying the companion of an extreme runaway massive binary

Melissa Munoz, Anthony F. J. Moffat, Grant M. Hill +5

WR 148 (HD 197406) is an extreme runaway system considered to be a potential candidate for a short-period (4.3173 d) rare WR + compact object binary. Provided with new high resolut…

astro-ph.SR2016★ 20 cited

An extensive spectroscopic time-series of three Wolf-Rayet stars. I. The lifetime of large-scale structures in the wind of WR 134

E. J. Aldoretta, N. St-Louis, N. D. Richardson +46

During the summer of 2013, a 4-month spectroscopic campaign took place to observe the variabilities in three Wolf-Rayet stars. The spectroscopic data have been analyzed for WR 134…