Observed epochal variations in X-ray lines from the O supergiant zeta Puppis do not require substantial changes in the wind mass flux

Sean J. Gunderson, Kenneth G. Gayley, David P. Huenemoerder, Pragati Pradhan, Nathan A. Miller

Research output: Contribution to journalArticlepeer-review

Original languageUndefined/Unknown
Pages (from-to)3154-3170
Number of pages17
JournalMonthly Notices of the Royal Astronomical Society
Volume529
Issue number4
DOIs
StatePublished - Apr 1 2024

Keywords

  • line: profiles
  • stars: massive
  • stars: mass-loss
  • stars: winds
  • outflows
  • X-rays: stars
  • Astrophysics - High Energy Astrophysical Phenomena
  • Astrophysics - Solar and Stellar Astrophysics

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