activity
19972023
most citedDiscovery of a magnetic field in the O9 sub-giant star HD 57682 by the MiMeS Collaboration

62 citations · 101 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.IM2023★ 2 cited

Addressing Outstanding Problems in the Physics of Massive Stars with the Line Emission Mapper X-ray Probe

Jeremy J. Drake, David Cohen, Michael Corcoran +5

We present some of the salient aspects of the scientific motivation for high resolution soft X-ray spectroscopy of early-type stars with the Line Emission Mapper X-ray Probe. The m…

astro-ph.SR2015★ 30 cited

First detections of 610 MHz radio emission from hot magnetic stars

P. Chandra, G. A. Wade, J. O. Sundqvist +7

We have carried out a study of radio emission from a small sample of magnetic O- and B-type stars using the Giant Metrewave Radio Telescope, with the goal of investigating their ma…

astro-ph.HE2012★ 7 cited

An X-ray Survey of Colliding Wind Binaries

Marc Gagne, Garrett Fehon, Michael Savoy +3

We have compiled a list of 36 O+O and 89 Wolf-Rayet binary candidates in the Milky Way and Magellanic clouds detected with the Chandra, XMM-Newton and ROSAT satellites to probe the…

astro-ph.SR2009★ 62 cited

Discovery of a magnetic field in the O9 sub-giant star HD 57682 by the MiMeS Collaboration

J. H. Grunhut, G. A. Wade, W. L. F. Marcolino +11

We report the detection of a strong, organised magnetic field in the O9IV star HD 57682, using spectropolarimetric observations obtained with ESPaDOnS at the 3.6-m Canada-France-Ha…

astro-ph2008

X-rays from magnetically channeled winds of OB stars

David H. Cohen

OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong and hard X-ray emission via the Magnetically Channeled Wind Shock (MCWS) mechani…

astro-ph2007

Quantitative analysis of resolved X-ray emission line profiles of O stars

David H. Cohen, Maurice A. Leutenegger, Richard H. D. Townsend

By quantitatively fitting simple emission line profile models that include both atomic opacity and porosity to the Chandra X-ray spectrum of Pup, we are able to explore the tra…