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[tel-00726959, v1] Caractériser le milieu interstellaire ... - HAL - INRIA

[tel-00726959, v1] Caractériser le milieu interstellaire ... - HAL - INRIA

[tel-00726959, v1] Caractériser le milieu interstellaire ... - HAL - INRIA

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254 ACTES DE COLLOQUES NATIONAUX ET INTERNATIONAUX<strong>tel</strong>-<strong>00726959</strong>, version 1 - 31 Aug 2012meier, & A. Heithausen, editor, The Dense Inters<strong>tel</strong>lar Medium in Galaxies, pages 521–+,2004.[C32] D. Teyssier, D. Fossé, M. Gerin, J. Pety, A. Abergel, and E. Habart. Connection BetweenPAHs and Small Hydrocarbons in the Horsehead Nebula PhotoDissociation Region. InC. L. Curry & M. Fich, editor, SFChem 2002 : Chemistry as a Diagnostic of Star Formation,pages 422–+, 2003.[C33] E. Falgarone, G. Pineau Des Forêts, P. Hily-Blant, P. Schilke, and J. Pety. NonequilibriumChemistry in the Dissipative Structures of Inters<strong>tel</strong>lar Turbu<strong>le</strong>nce. InC. L. Curry & M. Fich, editor, SFChem 2002 : Chemistry as a Diagnostic of Star Formation,pages 291–+, 2003.[C34] J. Pety, F. Gueth, S. Guilloteau, and A. Dutrey. The s<strong>tel</strong>lar mass of HH30. In F. Combes& D. Barret, editor, SF2A-2002 : Semaine de l’Astrophysique Francaise, pages 481–+,June 2002.[C35] J. Pety, F. Gueth, and S. Guilloteau. Simulating the wide-field imaging capabilities ofALMA. In F. Combes, D. Barret, & F. Thévenin, editor, SF2A-2001 : Semaine de l’AstrophysiqueFrancaise, pages 569–+, May 2001.[C36] E. Falgarone and J. Pety. Turbu<strong>le</strong>nce in the Environment of two Star<strong>le</strong>ss Dense Cores.In T. Montmer<strong>le</strong> & P. André, editor, From Darkness to Light : Origin and Evolution ofYoung S<strong>tel</strong>lar Clusters, volume 243 of Astronomical Society of the Pacific ConferenceSeries, pages 53–+, 2001.[C37] J. Pety and É. Falgarone. The structure of the cold neutral matter : shocks or vortices ? InYoung European Radio Astronomers’ Conference (YERAC), 2000.[C38] J. Pety and É. Falgarone. Kinematic localization of the dissipative structures of inters<strong>tel</strong>larturbu<strong>le</strong>nce. In Young European Radio Astronomers’ Conference (YERAC), 2000.[C39] D. C. Lis, T. G. Phillips, M. Gerin, J. Keene, Y. Li, J. Pety, and E. Falgarone. CentroidVelocity Increments as a Probe of the Turbu<strong>le</strong>nt Velocity Field in Inters<strong>tel</strong>lar Mo<strong>le</strong>cularClouds. In J. Franco & A. Carraminana, editor, Inters<strong>tel</strong>lar Turbu<strong>le</strong>nce, pages 203–+,1999.[C40] D. C. Lis, J. Pety, T. G. Phillips, and E. Falgarone. PDFs of centroid velocities andcentroid velocity increments in supersonic compressib<strong>le</strong> turbu<strong>le</strong>nce. In W. B. Latter,S. J. E. Radford, P. R. Jewell, J. G. Mangum, & J. Bally, editor, IAU Symposium, volume170 of IAU Symposium, pages 433–+, 1997.[C41] J. W. Kooi, J. Pety, P. L. Schaffer, T. G. Phillips, B. Bumb<strong>le</strong>, H. G. Leduc, and C. K.Walker. A 850 GHz SIS Receiver Employing Silicon Micro-Machining Technology. InE. J. Rolfe & G. Pilbratt, editor, Submillimetre and Far-Infrared Space Instrumentation,volume 388 of ESA Special Publication, pages 163–+, December 1996.

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