activity
20132022
most citedDetectability of small-scale magnetic fields in early-type stars

26 citations · 60 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2022★ 6 cited

Ultraviolet Spectropolarimetry With Polstar: Using Polstar to test Magnetospheric Mass-loss Quenching

M. E. Shultz, R. Casini, M. C. M. Cheung +17

Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution…

astro-ph.SR2022★ 7 cited

Ultraviolet Spectropolarimetric Diagnostics of Hot Star Magnetospheres

Asif ud-Doula, M. C. M. Cheung, A. David-Uraz +11

Several space missions and instruments for UV spectropolarimetry are in preparation, such as the proposed NASA MIDEX Polstar project, the proposed ESA M mission Arago, and the Poll…

astro-ph.IM2021

Ultraviolet Spectropolarimetry With Polstar: Hot Star Magnetospheres

M. E. Shultz, R. Casini, M. C. M. Cheung +17

Polstar is a proposed NASA MIDEX space telescope that will provide high-resolution, simultaneous full-Stokes spectropolarimetry in the far ultraviolet, together with low-resolution…

astro-ph.SR2017

Multiple, short-lived "stellar prominences" on the O giant Persei: a magnetic star?

N. Sudnik, H. F. Henrichs

We present strong evidence for a rotation period of 2.0406 d of the O giant Persei, derived from the NIV 1718 wind line in 12 yr of IUE data. We predict that Per has a m…

astro-ph.SR2016★ 15 cited

Multiple short-lived stellar prominences on O stars: The O6.5I(n)fp star lambda Cephei

N. P. Sudnik, H. F. Henrichs

Most O and many B stars show unexplained cyclical variability in their spectral lines, i.e. modulation on the rotational timescale, but not strictly periodic. The variability occur…

astro-ph.SR2013★ 6 cited

"Stellar Prominences" on OB stars to explain wind-line variability

H. F. Henrichs, N. P. Sudnik

Many O and B stars show unexplained cyclical variability in their winds, i.e. modulation of absorption features on the rotational timescale, but not strictly periodic over longer t…

astro-ph.SR2013★ 26 cited

Detectability of small-scale magnetic fields in early-type stars

O. Kochukhov, N. Sudnik

Strong, globally-organized magnetic fields are found for a small fraction of O, B, and A stars. At the same time, many theoretical and indirect observational studies suggested ubiq…