CONTAGIOUS B STAR FORMATION IN THE RHO OPHIUCHI DARK CLOUDFALGARONE E.1980; SYMP.-INT. ASTRON. UNION; ISSN 0074-1809; NLD; DA. 1980; NO 87; PP. 183-184; BIBL. 7 REF.Conference Paper

SOME OF THE PROBLEMS RAISED BY CO AND HCO⁺ OBSERVATIONS IN THE RHO OPHIUCHI CLOUDPERRAULT M; FALGARONE E.1981; ASTROPHYS. SPACE SCI. LIBR.; ISSN 0067-0057; NLD; DA. 1981; VOL. 93; PP. 315-321; BIBL. 8 REF.Conference Paper

Turbulence in interstellar cloudsFALGARONE, E.Lecture notes in physics. 1989, Vol 350, pp 68-79, issn 0075-8450Conference Paper

PARTIAL APERTURE SYNTHESIS OF FIVE DARK CLOUDS AT 1.4 GHZFALGARONE E; GILMORE W.1981; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1981; VOL. 95; NO 1; PP. 32-38; BIBL. 28 REF.Article

Structure at the 0.02 pc scale in molecular gas of low H₂ column densityFALGARONE, E; PERAULT, M.Astronomy and astrophysics (Berlin. Print). 1988, Vol 205, Num 1-2, pp L1-L4, issn 0004-6361Article

COLD MOLECULAR MATERIAL IN THE GALAXYEVANS NJ II; FEDERMAN SR; COMBES F et al.1982; SYMPOSIUM - INTERNATIONAL ASTRONOMICAL UNION; ISSN 0074-1809; NLD; DA. 1982; NO 100; PP. 45-46; BIBL. 5 REF.Conference Paper

CO OBSERVATIONS OF INTERSTELLAR CLOUDS: ISOTOPIC RATIOSCOMBES F; FALGARONE E; GUIBERT J et al.1980; ASTRON. ASTROPHYS. (BERL.); ISSN 0004-6361; DEU; DA. 1980; VOL. 90; NO 1-2; PP. 88-96; BIBL. 49 REF.Article

Model of clumped molecular clouds. II: Physics and evolution of the hierarchical structureFALGARONE, E; PUGET, J. L.Astronomy and astrophysics (Berlin. Print). 1986, Vol 162, Num 1-2, pp 235-247, issn 0004-6361Article

Structure and physics of cool giant molecular complexesFALGARONE, E; PERAULT, M.NATO ASI series. Series C, Mathematical and physical sciences. 1987, Vol 210, pp 59-73Conference Paper

Intermittency of interstellar turbulence: extreme velocity-shears and CO emission on milliparsec scaleFALGARONE, E; PETY, J; HILY-BLANT, P et al.Astronomy and astrophysics (Berlin. Print). 2009, Vol 507, Num 1, pp 355-368, issn 0004-6361, 14 p.Article

First detection of ¹³CH⁺ (J = 1-0)FALGARONE, E; PHILLIPS, T. G; PEARSON, John C et al.The Astrophysical journal. 2005, Vol 634, Num 2, pp L149-L152, issn 0004-637X, 2Article

The small-scale density and velocity structure of quiescent molecular cloudsFALGARONE, E; PUGET, J.-L; PERAULT, M et al.Astronomy and astrophysics (Berlin. Print). 1992, Vol 257, Num 2, pp 715-730, issn 0004-6361Article

Fragmented molecular clouds: statistical analysis of the ¹³CO(J = 1/0) emission distributionPERAULT, M; FALGARONE, E; PUGET, J. L et al.Astronomy and astrophysics (Berlin. Print). 1986, Vol 157, Num 1, pp 139-147, issn 0004-6361Article

Dissipative structures of diffuse molecular gas III. Small-scale intermittency of intense velocity-shearsHILY-BLANT, P; FALGARONE, E; PETY, J et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 481, Num 2, pp 367-380, issn 0004-6361, 14 p.Article

Fourier phase analysis in radio-interferometryLEVRIER, F; FALGARONE, E; VIALLEFOND, F et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 456, Num 1, pp 205-214, issn 0004-6361, 10 p.Article

CN Zeeman measurements in star formation regionsFALGARONE, E; TROLAND, T. H; CRUTCHER, R. M et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 487, Num 1, pp 247-252, issn 0004-6361, 6 p.Article

Einstein observations of the Rho Ophiuchi dark cloud: an X-ray Christmas treeMONTMERLE, T; KOCH-MIRAMOND, L; FALGARONE, E et al.The Astrophysical journal. 1983, Vol 269, Num 1, pp 182-201, issn 0004-637XArticle

X-ray variability of pre-main sequence objects associated with the Rho Oph dark cloudMONTMERLE, T; KOCH-MIRAMOND, L; FALGARONE, E et al.Physica scripta. T. 1984, Vol 7, pp 59-61, issn 0281-1847Article

Submillimeter observations of CO in Mars' atmosphereLELLOUCH, E; ENCRENAZ, T; PHILLIPS, T et al.Planetary and space science. 1991, Vol 39, Num 1-2, pp 209-212, issn 0032-0633, 4 p.Conference Paper

Jeans collapse of turbulent gas clouds : tentative theoryBONAZZOLA, S; PERAULT, M; PUGET, J. L et al.Journal of Fluid Mechanics. 1992, Vol 245, pp 1-28, issn 0022-1120Article

Molecular absorption lines toward star-forming regions: a comparative study of HCO⁺, HNC, HCN, and CNGODARD, B; FALGARONE, E; GERIN, M et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 520, issn 0004-6361, A20.1-A20.20Article

Warm gas in the cold diffuse interstellar medium : Spectral signatures in the H₂ pure rotational linesFALGARONE, E; VERSTRAETE, L; PINEAU DES FORETS, G et al.Astronomy and astrophysics (Berlin. Print). 2005, Vol 433, Num 3, pp 997-1006, issn 0004-6361, 10 p.Article

Jeans collapse in a turbulent mediumBONAZZOLA, S; FALGARONE, E; HEYVAERTS, J et al.Astronomy and astrophysics (Berlin. Print). 1987, Vol 172, Num 1-2, pp 293-298, issn 0004-6361Article

UV-driven chemistry in simulations of the interstellar medium I. Post-processed chemistry with the Meudon PDR codeLEVRIER, F; LE PETIT, F; HENNEBELLE, P et al.Astronomy and astrophysics (Berlin. Print). 2012, Vol 544, issn 0004-6361, A22.1-A22.13, 1Article

Large and small scale structures of molecular clouds in the Taurus Perseus complexFALGARONE, E; PUGET, J. L; EVANS, N. J et al.Lecture notes in physics. 1985, Num 237, pp 60-63, issn 0075-8450Article