Kinematic Be disk
The Kinematic Be disk model was created by A. Meilland.
It is described in the following article:
Kinematics and geometrical study of the Be stars 48 Persei and ψ Persei with the VEGA/CHARA interferometer
O. Delaa, Ph. Stee, A. Meilland, J. Zorec, D. Mourard, Ph. Bério, D. Bonneau, O. Chesneau, J. M. Clausse, P. Cruzalebes, K. Perraut, A. Marcotto, A. Roussel, A. Spang, H. McAlister, T. ten Brummelaar, J. Sturmann, L. Sturmann, N. Turner, C. Farrington and P. J. Goldfinger
A&A 529, A87 (2011)
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AMHRA's Kinematic Be disk service can be acknowledged by:
- And citing the article above.
Sample files are available for the following file fields: