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Observed epochal variations in X-ray lines from the O supergiant ζ Puppis do not require substantial changes in the wind mass flux
Sean J Gunderson, Kenneth G Gayley, David P Huenemoerder, Pragati Pradhan and Nathan A Miller Monthly Notices of the Royal Astronomical Society 529(4) 3154 (2024) https://doi.org/10.1093/mnras/stae547
Ultraviolet spectropolarimetric diagnostics of hot star magnetospheres
Correlated X-Ray and Optical Variability in the O-type Supergiant ζ Puppis
Joy S. Nichols, Yaël Nazé, David P. Huenemoerder, Anthony F. J. Moffat, Nathan A. Miller, Jennifer Lauer, Richard Ignace, Ken Gayley, Tahina Ramiaramanantsoa, Lidia Oskinova, Wolf-Rainer Hamann, Noel D. Richardson, Wayne L. Waldron and Matthew Dahmer The Astrophysical Journal 906(2) 89 (2021) https://doi.org/10.3847/1538-4357/abca3a
A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind
David P. Huenemoerder, Richard Ignace, Nathan A. Miller, Kenneth G. Gayley, Wolf-Rainer Hamann, Jennifer Lauer, Anthony F. J. Moffat, Yaël Nazé, Joy S. Nichols, Lidia Oskinova, Noel D. Richardson and Wayne Waldron The Astrophysical Journal 893(1) 52 (2020) https://doi.org/10.3847/1538-4357/ab8005
Chandra spectral measurements of the O supergiant ζ Puppis indicate a surprising increase in the wind mass-loss rate over 18 yr
David H Cohen, Jiaming Wang, Véronique Petit, et al. Monthly Notices of the Royal Astronomical Society 499(4) 6044 (2020) https://doi.org/10.1093/mnras/staa3124
Similar but different: the varied landscape of Onfp/Oef stars variability