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

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Contents I Foreword 13 1 15 II Executive Summary 17 1.1 Presentation of LAOG . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 1.1.1 A young, fast growing laboratory . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 1.1.2 Evolutions: scientific strategy and team synergy . . . . . . . . . . . . . . . . . . . . . . . 20 1.1.3 A brief overview of the scientific teams of LAOG . . . . . . . . . . . . . . . . . . . . . . . 24 1.1.4 Studentship at LAOG . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 1.1.5 Selected highlights and comparison with objectives of the previous report . . . . . . . . . 25 1.2 Bibliography . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27 1.3 Relations with the outside world . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28 1.3.1 Relations with and within the Observatory of Grenoble (OSUG) . . . . . . . . . . . . . . 28 1.3.2 Relations with IRAM . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 28 1.3.3 Relations with the University and with other local laboratories . . . . . . . . . . . . . . . 29 1.3.4 The European dimension of LAOG . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 29 1.3.5 Publicizing LAOG’s research: outreach and patents . . . . . . . . . . . . . . . . . . . . . 30 1.4 Budget: resources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 1.5 From dreams to reality: Human resources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 1.6 The 2007-2010 prospective and beyond . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 1.6.1 Main scientific objectives . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 34 1.6.2 Long-term strategic questions for LAOG . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37 1.7 Conclusions: A vision for the post-2010 future of LAOG . . . . . . . . . . . . . . . . . . . . . . . 38 5
Page 3: LABORATOIRE D’ASTROPHYSIQUE DE GR
Page 7 and 8: 4.4 The European Network “The Mol
Page 9 and 10: 11.3 Cameras and detectors . . . .
Page 11: 18.3 Equipment . . . . . . . . . .
Page 15: Chapter 1 The last Visiting Committ
Page 19 and 20: 1.1 Presentation of LAOG 1.1.1 A yo
Page 21 and 22: Figure 1.2: Old LAOG organigram (20
Page 23 and 24: Figure 1.4: The current repartition
Page 25 and 26: Permanent staff: 7. PhDs completed:
Page 27 and 28: - First fringes in the H band with
Page 29 and 30: clearly in its goals to have scient
Page 31 and 32: organization of astronomy events li
Page 33 and 34: • Contract-related funding. These
Page 35 and 36: in relation with planet formation.
Page 37 and 38: BASECOL database hosted in Meudon t
Page 39: exoplanetary atmospheres at LPG. Th
Page 43 and 44: Chapter 2 Presentation and Scientif
Page 45 and 46: supported by PCMI and PNPS, and mem
Page 47 and 48: (PV) are also involved in several h
Page 49 and 50: Chapter 3 Results 3.1 Overview In t
Page 51 and 52: et al. 2002, 2003). When CO disappe
Page 53 and 54: 3.2.4 The outflows of protostars As
Page 55 and 56:
Since X-rays mainly come from flare
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• Monitoring of the error propaga
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Rate coefficient (cm 3 s -1 ) 1e-10
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Differential Cross Section (Å 2 sr
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Figure 3.7: Detection of HDO in the
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Chapter 4 Perspectives 4.1 Overview
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in the midplane of young disks surr
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more difficult (iv) The region wher
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• 12D-Surface of NH3 with H2 •
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for doing that, but we are limited
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• Determination of the gas-to-dus
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Chapter 6 Introduction of the team
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the central star. They regulate the
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disks. At these wavelength, the bul
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Wind and disk interaction in MWC 29
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6.3.3 The physics and origins of ma
Page 89 and 90:
Figure 6.5: Observation and model o
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Multiplicity of protostars Followin
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masses up to 10 solar masses for a
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Figure 6.9: Top panels: DENIS disco
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process by comparing its outcome fo
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With this new tool at hands, search
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Chapter 7 Future Research Direction
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at LAOG (in collaboration with Gene
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8.1.3 Graduate Students Completed P
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Part V TEAM GRIL The first fringes
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Chapter 9 Presentation of the team
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Chapter 10 Scientific rationale 10.
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The first and last items are a defi
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Figure 10.1: The logical link betwe
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Figure 11.1: NAOS-CONICA installed
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Figure 11.3: Left: the first 52-act
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Figure 11.4: Left: the AMBER instru
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Figure 11.6: Left: Integrated optic
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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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¡ ¢£¤¥¦§¨¤¥©¢£�§¨
Page 183:
20.15 Prospective Le centre Mariott
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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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