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 BrummelaarH.~A. McAlister, N.~H. Turner, J. Sturmann, L. Sturmann, S.~T. Ridgway

Research output: Contribution to journalArticlepeer-review

21 Citations (Scopus)
Original languageEnglish
Pages (from-to)A59
Number of pages15
JournalAstronomy and Astrophysics
Volume545
DOIs
Publication statusPublished - 1 Sep 2012

Keywords

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

Cite this