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The relationship between γ Cassiopeiae's X-ray emission and its circumstellar environment. II. Geometry and kinematics of the disk from MIRC and VEGA instruments on the CHARA Array

  • P. Stee
  • , O. Delaa
  • , J.~D. Monnier
  • , A. Meilland
  • , K. Perraut
  • , D. Mourard
  • , X. Che
  • , G.~H. Schaefer
  • , E. Pedretti
  • , M.~A. Smith
  • , R. Lopes de Oliveira
  • , C. Motch
  • , G.~W. Henry
  • , N.~D. Richardson
  • , K.~S. Bjorkman
  • , R. Bücke
  • , E. Pollmann
  • , J. Zorec
  • , D.~R. Gies
  • , T. ten Brummelaar
  • H.~A. McAlister, N.~H. Turner, J. Sturmann, L. Sturmann, S.~T. Ridgway

Research output: Contribution to journalArticlepeer-review

Original languageEnglish
Article numberA59
JournalAstronomy and Astrophysics
Volume545
DOIs
Publication statusPublished - Sept 2012

Keywords

  • techniques: interferometric, stars: emission-line, Be, stars: winds, outflows, circumstellar matter, binaries: close

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