Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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Part IV TEAM FOST The first image of a planetary mass companion outsi<strong>de</strong> our solar system, observed with NAOS on the VLT 77
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LABORATOIRE D’ASTROPHYSIQUE DE GR
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III Team ASTROMOL 41 2 Presentation
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8.1.3 Graduate Students . . . . . .
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VI Team SHERPA 145 15 Results 147 1
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Part I Foreword: Presentation of th
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Part II Executive Summary A 18th ce
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of CNRS for technicians and enginee
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Figure 1.3: New LAOG organigram (20
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heart attack. Manuel went back to t
Page 26 and 27: Figure 1.6: PhD student repartition
Page 28 and 29: • LAOG researchers (and publishin
Page 30 and 31: and published 95 papers in four yea
Page 32 and 33: • National astronomy programs. 4
Page 34 and 35: 1.5 From dreams to reality: Human r
Page 36 and 37: and accretion disks with heavy nume
Page 38 and 39: emphasis on the chemistry of planet
Page 41: Part III TEAM ASTROMOL Sub-arcsecon
Page 44 and 45: • we develop quantum and classica
Page 46 and 47: Table shows not only the volume of
Page 48 and 49: • Herschel-HIFI: Astromol is invo
Page 50 and 51: particular, we calculated a 9D H2O-
Page 52 and 53: • The hot corinos. More spectacul
Page 54 and 55: the massive deeply embedded protost
Page 56 and 57: tens of visual magnitudes, hence pr
Page 58 and 59: quantum VCC-IOS approximation may f
Page 60 and 61: Rate constant (cm 3 s -1 ) 1e-09 1e
Page 62 and 63: • One of us (PV) is strongly invo
Page 64 and 65: sublimation of water ice trapped ei
Page 66 and 67: If the chemistry in the first phase
Page 68 and 69: 4.2.2 Molecular Physics The theoret
Page 70 and 71: Source Herschel Time Astromol Class
Page 72 and 73: several important studies that anti
Page 74 and 75: Chapter 5 Selected Publications •
Page 79 and 80: Chapter 6 Introduction of the team
Page 81 and 82: the central star. They regulate the
Page 83 and 84: disks. At these wavelength, the bul
Page 85 and 86: Wind and disk interaction in MWC 29
Page 87 and 88: 6.3.3 The physics and origins of ma
Page 89 and 90: Figure 6.5: Observation and model o
Page 91 and 92: Multiplicity of protostars Followin
Page 93 and 94: masses up to 10 solar masses for a
Page 95 and 96: Figure 6.9: Top panels: DENIS disco
Page 97 and 98: process by comparing its outcome fo
Page 99 and 100: With this new tool at hands, search
Page 101 and 102: Chapter 7 Future Research Direction
Page 103 and 104: at LAOG (in collaboration with Gene
Page 105 and 106: 8.1.3 Graduate Students Completed P
Page 107 and 108: Part V TEAM GRIL The first fringes
Page 109 and 110: Chapter 9 Presentation of the team
Page 111 and 112: Chapter 10 Scientific rationale 10.
Page 113 and 114: The first and last items are a defi
Page 115 and 116: Figure 10.1: The logical link betwe
Page 117 and 118: Figure 11.1: NAOS-CONICA installed
Page 119 and 120: Figure 11.3: Left: the first 52-act
Page 121 and 122: Figure 11.4: Left: the AMBER instru
Page 123 and 124: Figure 11.6: Left: Integrated optic
Page 125 and 126: Figure 11.8: Left panel: Process fl
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Figure 11.9: Left View of the WIRCa
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Chapter 12 Perspectives The instrum
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12.1.2 R&D activities PRIORITIES Fo
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laboratories of OSUG, a collaborati
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collaborations. Moreover, part of o
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Chapter 13 Recruitment plan GRIL ne
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Chapter 14 Appendix 14.1 Staff 14.1
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• Tantalum superconducting tunnel
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• I3 IInternational Integrating I
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Part VI TEAM SHERPA The two-flow pa
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Chapter 15 Results 15.1 History and
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Figure 15.1: A standard accretion d
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mechanics community, for non-rotati
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to be produced in the relativistic
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Figure 15.3: The spectrum of cosmic
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Ferreira, in collaboration with Ron
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• “Particle Transport in Tangle
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controls the level of the anomalous
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Part VII APPENDICES 163
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Chapter 17 Appendix 1: General orga
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Chapter 18 Appendix 2: LAOG Technic
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Chapter 19 Appendix 3: Internationa
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19.2 Organisation de colloques, wor
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(2003-présent): Membre du CNAP, se
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Membre du conseil scientifique du L
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• LESIA (Observatoire de Paris-Me
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20.9 Groupes de Recherche et Dével
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20.15 Prospective Le centre Mariott
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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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