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20072009
most citedDynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: II. The Effects of Field-Aligned Rotation

254 citations · 783 across the 8 of their papers we have counts for

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astro-ph2008

Angular Momentum Loss and Stellar spin-down in Magnetic Massive Stars

Asif ud-Doula, Stanley P. Owocki, Richard H. D. Townsend

We examine the angular momentum loss and associated rotational spin-down for magnetic hot stars with a line-driven stellar wind and a rotation-aligned dipole magnetic field. Our an…

astro-ph2008252 cited

Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: III. Angular Momentum Loss and Rotational Spindown

Asif ud-Doula, Stanley P. Owocki, Richard H. D. Townsend

We examine the angular momentum loss and associated rotational spindown for magnetic hot stars with a line-driven stellar wind and a rotation-aligned dipole magnetic field. Our ana…

astro-ph200843 cited

Exploring the photometric signatures of magnetospheres around Helium-strong stars

R. H. D. Townsend

The photometric variations due to magnetically confined material around He-strong stars are investigated within the framework of the Rigidly Rotating Magnetosphere (RRM) model. For…

astro-ph200817 cited

The most rapidly rotating He-strong emission line star: HR7355

Th. Rivinius, S. Stefl, R. H. D. Townsend +1

Using archival spectroscopic and photometric data, we searched for massive stars with Balmer-emission consistent with magnetically confined circumstellar material. HR 7355 is a for…

astro-ph2007254 cited

Dynamical Simulations of Magnetically Channeled Line-Driven Stellar Winds: II. The Effects of Field-Aligned Rotation

Asif ud-Doula, Stanley Owocki, Richard Townsend

Building upon our previous MHD simulation study of magnetic channeling in radiatively driven stellar winds, we examine here the additional dynamical effects of stellar {\em rotatio…

astro-ph20078 cited

The coupling between pulsation and mass loss in massive stars

Rich Townsend

To what extent can pulsational instabilities resolve the mass-loss problem of massive stars? How important is pulsation in structuring and modulating the winds of these stars? What…