A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind
Author:
Funder
Smithsonian Astrophysical Observatory
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab8005/pdf
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1. Survey of X-Rays from Massive Stars Observed at High Spectral Resolution with Chandra;The Astrophysical Journal;2023-08-29
2. Support for the standard picture of thermal X-rays in the wind of ζ Puppis from dielectronic recombination of He-like ions;Monthly Notices of the Royal Astronomical Society;2023-04-20
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4. Helium-like X-ray line complexes show that the hottest plasma on the O supergiant ζ Puppis is in its wind;Monthly Notices of the Royal Astronomical Society;2022-04-05
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