BRITE-Constellation high-precision time-dependent photometry of the early O-type supergiant zeta Puppis unveils the photospheric drivers of its small- and large-scale wind structures

Tahina Ramiaramanantsoa, Anthony F.~J. Moffat, Robert Harmon, Richard Ignace, Nicole St-Louis, Dany Vanbeveren, Tomer Shenar, Herbert Pablo, Noel D. Richardson, Ian D. Howarth, Ian R. Stevens, Caroline Piaulet, Lucas St-Jean, Thomas Eversberg, Andrzej Pigulski, Adam Popowicz, Rainer Kuschnig, Elżbieta Zocłońska, Bram Buysschaert, Gerald HandlerWerner W. Weiss, Gregg A. Wade, Slavek M. Rucinski, Konstanze Zwintz, Paul Luckas, Bernard Heathcote, Paulo Cacella, Jonathan Powles, Malcolm Locke, Terry Bohlsen, André-Nicolas Chené, Brent Miszalski, Wayne L. Waldron, Marissa M. Kotze, Enrico J. Kotze, Torsten Böhm

Research output: Contribution to journalArticlepeer-review

Original languageUndefined/Unknown
Pages (from-to)5532-5569
Number of pages38
JournalMonthly Notices of the Royal Astronomical Society
Volume473
Issue number4
DOIs
StatePublished - Feb 1 2018

Keywords

  • techniques: photometric
  • techniques: spectroscopic
  • stars: massive
  • stars: rotation
  • starspots
  • supergiants
  • stars: winds
  • outflows
  • Astrophysics - Solar and Stellar Astrophysics

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