The Infrared Space Observatory (ISO) was launched on November 17 1995 and has been operated successfully since then. As the first results have already shown, ISO has provided a breakthrough in our understanding of the composition of cosmic gas and dust, the physical processes related to star formation, the evolution of stars in both our and external galaxies, the mechanisms at play in the infrared galaxies and the nature of their powering sources up to cosmological distances. The infrared observations provided by ISO connect many fields of astronomy through the diagnostics of the major atomic and molecular cooling lines or important physical processes like the dust/gas exchange and the chemistry.
By the autumn of 1998, half a year after the end of the mission, many results will be available and ready for presentation. Thus, it appears appropriate at that time to hold a major scientific meeting to summarise and discuss the results obtained during the ISO mission in all fields of astrophysics.
Name | Institute |
---|---|
M.E. Anderegg | ESA/ESTEC, Noordwijk, NL |
E. Becklin | University of California, Los Angeles, USA |
J. Cernicharo | Instituto de Estructura de la Materia, Madrid, Spain |
C. Cesarsky - Chair | CEA-Saclay, Gif-sur-Yvette, F |
P.E. Clegg | Queen Mary and Westfield College, London, UK |
P. Cox | Institut d'Astrophysique Spatiale, Orsay, F |
Th. Encrenaz | Observatoire de Paris-Meudon, Meudon, F |
R. Genzel | MPI fuer Extraterrestrische Physik, Garching, D |
Th. De Graauw | SRON, Groningen, NL |
H. J. Habing | Sterrewacht, Leiden, NL |
M. Harwit | Washington, USA |
G. Helou | IPAC, Pasadena, USA |
D. Hollenbach | NASA/Ames, Moffet Field, USA |
M.F. Kessler | ESA, Villafranca, Spain |
D. Lemke | Max-Planck-Institut fuer Astronomie, Heidelberg, D |
A.F. Moorwood | ESO, Garching, D |
A. Natta | Osservatorio di Arcetri, Firenze, I |
L. Nordh | Stockholm Observatory, Stockholm, Sweden |
H. Okuda | ISAS, Kanagawa, Japan |
J.L. Puget - Co-chair | Institut d'Astrophysique Spatiale, Orsay, F |
M. Rowan-Robinson | Imperial College, London, UK |
T. Tsuji | Institute of Astronomy, Tokyo, Japan. |
Name | Institute |
---|---|
P.Cox - Chair | Institut d'Astrophysique Spatiale, Orsay, F |
V. Demuyt - Secretary | Institut d'Astrophysique Spatiale, Orsay, F |
Th. Encrenaz | Observatoire de Paris-Meudon, Meudon, F |
M. Joubert | CNES, Toulouse, F |
L. Vigroux | Saclay-CEA, F |
S. Volonte | ESA/Scientific Programme Directorate, Paris, F |
Confirmed invited speakers include:
S. Beckwith, C. Cesarsky, P.E. Clegg, T. de Graauw, B. Draine, E. Dwek, D. Elbaz, R. Genzel, M. Harwit, G. Helou, M. Kessler, E. Lellouch, D. Lemke, A. Moorwood, P. Morris, A. Omont, J.-L. Puget, E. van Dishoeck, C. Waelkens.
Papers for presentation will be selected on the basis of abstracts of approximately 300-500 words. The abstract should clearly outline the paper's major elements of interest and its originality. Papers will be selected on the basis of:
Abstracts should contain the following information:
Abstracts should be sent by e-mail before 15 May 1998 to 'isoconf@ias.fr'
Authors will be notified of the decision of the Programme Committee by 1 July 1998. Authors whose paper has been accepted will then receive the necessary instructions for the preparation of their manuscript.
March 1998 | Second Announcement: This will contain information on logistics (hotels, venue, etc..) |
15 May 1998 | Deadline for submission of a one-page abstract |
1 July 1998 | Notification of acceptance and issue of instructions for submission of papers to authors |
1 July 1998 | Preliminary Programme on WWW |
September 1998 | Registration deadline |
20-23 October | Conference |
December 1998 | Publication of Proceedings |
/isoconf@ias.fr
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