activity
19972012
most citedChandra Discovers a Very High Density X-ray Plasma on the O-Star Zeta Orionis

131 citations · 1.1k across the 27 of their papers we have counts for

collaborators

26 papers

astro-ph.SR2012★ 15 cited

X-ray Emission Line Profiles from Wind Clump Bow Shocks in Massive Stars

R. Ignace, W. L. Waldron, J. P. Cassinelli

The consequences of structured flows continue to be a pressing topic in relating spectral data to physical processes occurring in massive star winds. In a preceding paper, our grou…

astro-ph.SR2011★ 118 cited

Early magnetic B-type stars: X-ray emission and wind properties

L. M. Oskinova, H. Todt, R. Ignace +3

We present a comprehensive study of X-ray emission and wind properties of massive magnetic early B-type stars. Dedicated XMM-Newton observations were obtained for three stars xi1 C…

astro-ph.IM2011★ 9 cited

Time-Dependent Behavior of Linear Polarization in Unresolved Photospheres, With Applications for The Hanle Effect

R. Ignace, K. T. Hole, J. P. Cassinelli +1

Aims: This paper extends previous studies in modeling time varying linear polarization due to axisymmetric magnetic fields in rotating stars. We use the Hanle effect to predict var…

astro-ph.SR2010★ 21 cited

A Multi-Phase Suzaku Study of X-rays from tau Sco

R. Ignace, L. M. Oskinova, M. Jardine +5

We obtained relatively high signal-to-noise X-ray spectral data of the early massive star tau Sco (B0.2V) with the Suzaku XIS instrument. This source displays several unusual featu…

astro-ph.SR2009★ 10 cited

Polarization Variability Arising from Clumps in the Winds of Wolf-Rayet Stars

Q. Li, J. P. Cassinelli, J. C. Brown +1

The polarimetric and photometric variability of Wolf-Rayet (WR) stars as caused by clumps in the winds, is revisited. In the model which is improved from Li et al. 2000, the radial…

astro-ph2008★ 14 cited

Protodiscs around Hot Magnetic Rotator Stars

M. Maheswaran, J. P. Cassinelli

We develop equations and obtain solutions for the structure and evolution of a protodisc region that is initially formed with no radial motion and super-Keplerian rotation speed wh…