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Evry SCHATZMAN Radio-Astronomie, E. N. S. , Paris, France The
recent developments of the Supernova theory and numerical
relativity can lead in the near future to an understanding of
gravitational collapse and to a reliable prediction of the
amplitude of the gravitational waves generated during neutron star
formation. These prospects explain the great interest which has
developed in the international scientific community for the
workshop. We were financially limited in the number of guests and
participants and we apologize for not having been able to gather
all the specialists actually involved in research programs relevant
to gravitational collapse and numerical relativity. This limitation
took place despite all the financial assistance which we have
received from various institutions, first the C. N. R. S. (Centre
National de 1a Recherche Scientifique) which has supported the
request of Dr. Monique SIGNORE of organizing a workshop. Furhter
help was obtained from I. N. A. G. (Institut National d'Astronomie
et de Geophysique), Toulouse University (Universite "Paul Sabatier"
or "Toulouse III"), the Toulouse section of C. N. E. S. (Centre
National d'Etudes Spatia1es), the Department of theoretical physics
of the C. E. A. , the Department of Astrophysique of the C. E. A.
(Centre d'Etudes Nucleaires, Saclay), D. R. E. T. (Direction des
Recherches Etudes et Techniques) and last but not least an
important grant from NATO, whose scientific Committee recognized
the international significance of the workshop. The meeting was
organized by Professor D.
Evry SCHATZMAN Radio-Astronomie, E. N. S. , Paris, France The
recent developments of the Supernova theory and numerical
relativity can lead in the near future to an understanding of
gravitational collapse and to a reliable prediction of the
amplitude of the gravitational waves generated during neutron star
formation. These prospects explain the great interest which has
developed in the international scientific community for the
workshop. We were financially limited in the number of guests and
participants and we apologize for not having been able to gather
all the specialists actually involved in research programs relevant
to gravitational collapse and numerical relativity. This limitation
took place despite all the financial assistance which we have
received from various institutions, first the C. N. R. S. (Centre
National de 1a Recherche Scientifique) which has supported the
request of Dr. Monique SIGNORE of organizing a workshop. Furhter
help was obtained from I. N. A. G. (Institut National d'Astronomie
et de Geophysique), Toulouse University (Universite "Paul Sabatier"
or "Toulouse III"), the Toulouse section of C. N. E. S. (Centre
National d'Etudes Spatia1es), the Department of theoretical physics
of the C. E. A. , the Department of Astrophysique of the C. E. A.
(Centre d'Etudes Nucleaires, Saclay), D. R. E. T. (Direction des
Recherches Etudes et Techniques) and last but not least an
important grant from NATO, whose scientific Committee recognized
the international significance of the workshop. The meeting was
organized by Professor D.
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