The scientific crew of the Flying Saucer
The Flying Saucer protoplanetary disk is studied by a large international consortium comprised of scientists from Europe, United States, and East Asia. The overall structure of the consortium and the division of scientific labors is presented in the following scheme:
Management
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Level 1 |
Data Reduction & Delivers |
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IRAM: E. Chapillon Data Reduction & Archive Distribution to EU |
ASIAA: Y. W. Tang |
RICE: A. Isella Data Reduction & Archive Distribution to NA |
ESO: L. Testi Image Processing Distribution |
Level 2 |
Observational Interpretation |
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Observational Model |
Line Radiative Transder & Thermal Structure NASA Ames: U. Gorti |
Simpel Dust Model RICE University: A. Isella |
Multi- lambda Obs. Strasbourg: N. Grosso |
Level 3 |
Comparison to Numerical Models, Young Solar Systems & exo-planet synthesis |
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Chemical Models: MPIA D. Semenov |
2D / 3D Dust structure & evolution MPIA: T. Birnstiel |
Dynamics of Gas and Dust, Turbulence Obs. Nice: H. Meheut |
Project coordinators:
Anne Dutrey (Laboratoire d'Astrophysique de Bordeaux, France)
Paul Ho (Academia Sinica, Institute of Astronomy and Astrophysics, Taiwan)
Level 1: Data Reduction & Delivery
Edwige Chapillon (LAB, IRAM, France)
Andrea Isella (Rice University, Houston, TX, USA)
Vincent Piétu (Institut de Radio-Astronomie Millimétrique (IRAM), Grenoble, France)
Ya-Wen Tang (ASIAA, Academia Sinica, Taiwan)
Leonardo Testi (ESO, Garching bei Muenchen, Germany)
Others: A. Dutrey, P. Ho, St. Guilloteau, Y. Boehler, P.Y. Hieh, M.Tazzari, F. Gueth, P. Gratier, A. Kospal
Level 2: Observational Interpretation
Observational model:
Yann Boehler (Rice University, Houston, TX, USA)
Stephane Guilloteau (Laboratoire d'Astrophysique de Bordeaux, France)
Others: A. Isella, L. Testi, M. Tazzari, A. Dutrey, E. Di Folco, P.G. Du, J. Cuzzi, Y.-W. Tang
Simple dust models:
Marco Tazzari (European Southern Observatory, Germany)
Sebastian Wolf (Kiel University, Germany)
Multi-wavelength observations:
Nicolas Grosso (Observatoire Astronomique de Strasbourg, France)
Michihiro Takami (Institute of Astronomy and Astrophysics, Academia Sinica Taiwan)
Karl Stapelfeldt (Jet Propulsion Laboratory, Caltech, USA)
Others: S. Wolf, D. Padgett, M. Takami, E. Di Folco
Line radiative transfer models:
Uma Gorti (SETI Institute, Mountin View, USA)
Richard Teague (Max Planck Institute for Astronomy, Heidelberg, Germany)
Others: I. Cleeves, Y. Pavlyuchenkov, St. Guilloteau, A. Dutrey, A. Isella, S.Y. Liu, A. Kospal
Level 3: Theoretical models
Disk turbulence and hydrodynamics:
Héloïse Méheut (Observatoire de la Côte d'Azur, France)
Others: St. Guilloteau, A. Dutrey, R. Teague, J. Cuzzi, H. Meheut, S. Fromang, U. Gorti, Th. Henning, F. Hersant, A.Pierens, M.Bate, S.Fromang, W.K.Lee
Disk dust evolution:
Tilman Birnstiel (Max Planck Institute for Astronomy, Heidelberg, Germany)
Akimasa Kataoka (Heidelberg University, Germany)
Satoshi Okuzumi (Tokyo Institute of Technology, Japan)
Others: C. Dullemond, Ch. Ormel, T. Guillot, Th. Henning, S.Ida
Disk chemistry evolution:
Yuri Aikawa (Center for Computational Sciences, University of Tsukuba, Japan)
Edwin Bergin (University of Michigan, Ann Arbor, USA)
Ilse Cleeves (CfA, USA)
Pierre Gratier (Laboratoire d’Astrophysique de Bordeaux, France)
Frank Hersant (Laboratoire d’Astrophysique de Bordeaux, France)
Liton Majumdar (Laboratoire d’Astrophysique de Bordeaux, France)
Dmitry Semenov (Max Planck Institute for Astronomy, Heidelberg, Germany)
Valentine Wakelam (Laboratoire d’Astrophysique de Bordeaux, France)
Karen Willacy (NASA/JPL, USA)
Others: D. Wiebe, A. Vasyunin
Link to solar system and exoplanet synthesis:
Aurélien Crida (Lagrange (UCA/OCA), IUF, France)
Tristan Guillot (Lagrange (UCA/OCA), IUF, France)
Thomas Henning (Max Planck Institute for Astronomy, Heidelberg, Germany)
Christoph Mordasini (Physics Institute, University of Bern, Switzerland)
Others: H.Meheut, A. Morbidelli, M. Bate, K. Willacy, S. Ida, S. Okuzumi