activity
20022023
most citedThe MiMeS Survey of Magnetism in Massive Stars: Introduction and overview

232 citations · 3.4k across the 140 of their papers we have counts for

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Showing 2016Show all

7 papers · 1 filter

astro-ph.SR2016★ 8 cited

The BRITE spectropolarimetric program

Coralie Neiner, Gregg Wade, Stephen Marsden +1

A high-resolution spectropolarimetric survey of all (573) stars brighter than magnitude V=4 has been undertaken with Narval at TBL, ESPaDOnS at CFHT, and HarpsPol at ESO, as a grou…

astro-ph.SR2016

Understanding the photometric variability of ζ Ori Aa

B. Buysschaert, C. Neiner, T. Ramiaramanantsoa +3

We studied the variability of the magnetic O-type supergiant Ori Aa using multi-colour BRITE photometry. We confirmed the known rotation frequency …

astro-ph.SR2016★ 2 cited

The puzzling properties of the magnetic O star Tr16-22

Yael Naze, Rodolfo Barba, Stefano Bagnulo +4

(abridged version) Context : The detection of bright, hard, and variable X-ray emission in Tr16-22 prompted spectropolarimetric observations of this star, which in turn led to the…

astro-ph.SR2016★ 25 cited

HD 35502: a hierarchical triple system with a magnetic B5IVpe primary

James Sikora, Gregg Wade, David Bohlender +8

We present our analysis of HD~35502 based on high- and medium-resolution spectropolarimetric observations. Our results indicate that the magnetic B5IVsnp star is the primary compon…

astro-ph.SR2016★ 41 cited

Discovery of a very weak magnetic field on the Am star Alhena

Aurore Blazère, Coralie Neiner, Pascal Petit

Alhena ( Gem) was observed in the frame of the BRITE (BRIght Target Explorer) spectropolarimetric survey, which gathers high resolution, high signal-to-noise, high sensitivity,…

astro-ph.SR2016★ 12 cited

Weak magnetic field, solid-envelope rotation, and wave-induced N-enrichment in the SPB star Cassiopeiae

M. Briquet, C. Neiner, P. Petit +3

Aims. The main-sequence B-type star Cassiopeiae is known as a N-rich star with a magnetic field discovered with the Musicos spectropolarimeter. We model the magnetic field of t…