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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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ARTICLES PUBLIÉS DANS DES REVUES À COMITÉ DE LECTURE 247<strong>tel</strong>-<strong>00726959</strong>, version 1 - 31 Aug 2012[A25] J. R. Goicoechea, J. Pety, M. Gerin, D. Teyssier, E. Roueff, P. Hily-Blant, and S. Baek.Low sulfur dep<strong>le</strong>tion in the Horsehead PDR. A&A, 456 :565–580, September 2006.[A26] S. Cabrit, J. Pety, N. Pesenti, and C. Dougados. Tidal stripping and disk kinematics inthe RW Aurigae system. A&A, 452 :897–906, June 2006.[A27] H. S. Liszt, R. Lucas, and J. Pety. Comparative chemistry of diffuse clouds. V. Ammoniaand formaldehyde. A&A, 448 :253–259, March 2006.[A28] E. Habart, A. Abergel, C. M. Walms<strong>le</strong>y, D. Teyssier, and J. Pety. Density structure of theHorsehead nebula photo-dissociation region. A&A, 437 :177–188, July 2005.[A29] J. Pety, D. Teyssier, D. Fossé, M. Gerin, E. Roueff, A. Abergel, E. Habart, and J. Cernicharo.Are PAHs precursors of small hydrocarbons in photo-dissociation regions ? TheHorsehead case. A&A, 435 :885–899, June 2005.[A30] J. Pety, A. Bee<strong>le</strong>n, P. Cox, D. Downes, A. Omont, F. Bertoldi, and C. L. Carilli. Atomiccarbon in PSS 2322+1944, a quasar at redshift 4.12. A&A, 428 :L21–L24, December 2004.[A31] A. Bee<strong>le</strong>n, P. Cox, J. Pety, C. L. Carilli, F. Bertoldi, E. Momjian, A. Omont, P. Petitjean,and A. O. Petric. Starburst activity in the host galaxy of the z =2.58 quasar J1409+5628.A&A, 423 :441–447, August 2004.[A32] D. Teyssier, D. Fossé, M. Gerin, J. Pety, A. Abergel, and E. Roueff. Carbon budget andcarbon chemistry in Photon Dominated Regions. A&A, 417 :135–149, April 2004.[A33] J. Pety and E. Falgarone. Non-Gaussian velocity shears in the environment of low massdense cores. A&A, 412 :417–430, December 2003.[A34] P. Cox, A. Omont, S. G. Djorgovski, F. Bertoldi, J. Pety, C. L. Carilli, K. G. Isaak, A. Bee<strong>le</strong>n,R. G. McMahon, and S. Castro. CO and Dust in PSS 2322+1944 at a redshift of 4.12.A&A, 387 :406–411, May 2002.[A35] E. Falgarone, J. Pety, and T. G. Phillips. Filamentary Structure and Helical MagneticFields in the Environment of a Star<strong>le</strong>ss Dense Core. ApJ, 555 :178–190, July 2001.[A36] J. Pety and É. Falgarone. The elusive structure of the diffuse mo<strong>le</strong>cular gas : shocks orvortices in compressib<strong>le</strong> turbu<strong>le</strong>nce ? A&A, 356 :279–286, April 2000.[A37] J. W. Kooi, J. Pety, B. Bumb<strong>le</strong>, C. K. Walker, H. G. Leduc, P. L. Schaffer, and T. G.Phillips. A 850-GHz waveguide receiver employing a niobium SIS junction fabricated on a1-µm Si/sub 3/N/sub 4/ membrane. IEEE Transactions on Microwave Theory Techniques,46 :151–161, February 1998.[A38] D. C. Lis, J. Keene, Y. Li, T. G. Phillips, and J. Pety. Statistical Properties of LineCentroid Velocity Increments in the rho Ophiuchi Cloud. ApJ, 504 :889–+, September1998.[A39] D. C. Lis, J. Pety, T. G. Phillips, and E. Falgarone. Statistical Properties of Line CentroidVelocities and Centroid Velocity Increments in Compressib<strong>le</strong> Turbu<strong>le</strong>nce. ApJ, 463 :623–+, June 1996.[A40] J.-C. Maréchal, J. Pety, Y. Simon, and M. David. Analytical comparison of differenttypes of pulse tubes refrigerators. Cryogenics, 34 :163–166, 1994.

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