The relationship between gamma 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 Article (Web of Science)

International Collaboration

cited authors

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

publication date

  • September 1, 2012


published in

author keyword

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



  • 545