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

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VI Team SHERPA 145 15 Results 147 15.1 History and group composition . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 15.2 Specific approach . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 147 15.3 Accretion-Ejection . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148 15.3.1 The self-similar model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 148 15.3.2 Application to different astrophysical contexts . . . . . . . . . . . . . . . . . . . . . . . . . 148 15.4 Transport phenomena in accretion-ejection flows . . . . . . . . . . . . . . . . . . . . . . . . . . . 150 15.4.1 Jet stability . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 150 15.4.2 Transport in accretion disks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 150 15.5 Physics of high energy sources . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 151 15.5.1 Seyfert galaxies . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 151 15.5.2 Blazars and the “two-flow” model . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 152 15.5.3 Microquasars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 153 15.6 Relativistic Plasmas and Cosmic Rays . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 15.6.1 Relativistic plasmas . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 15.6.2 Cosmic Rays . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 154 15.7 Heavy numerical simulations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 156 15.8 Astrocladistics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 15.9 Participation in large collaborations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 157 15.10 Doctoral formation and Schools . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158 15.11 Scientific Highlights (2002-2005) . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 158 16 Perspectives 160 VII APPENDICES 163 17 Appendix 1: General organization of LAOG 165 17.1 Management structure . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 165 17.2 Management tools and quality control . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 166 18 Appendix 2: LAOG Technical group & facilities 167 18.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 167 18.2 Teams . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 167 10
18.3 Equipment . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 168 19 Appendix 3: Staff Responsabilities 169 19.1 International . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169 19.1.1 Astromol . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169 19.1.2 FOST . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 169 19.1.3 GRIL . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170 19.1.4 SHERPA . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 170 19.2 Workshops . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171 19.2.1 FOST . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171 19.3 National . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171 19.3.1 Astromol . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 171 19.3.2 FOST . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 172 19.3.3 GRIL . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 173 19.3.4 SHERPA . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 174 20 Appendix 4: The Jean Marie Mariotti Center 176 20.1 Mission . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 176 20.2 Structure . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 176 20.3 Statut . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177 20.4 Budget . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177 20.5 Direction et personnel . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177 20.6 Le centre de réalisation logicielle . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 177 20.7 Production informatique . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 20.8 Organisation de services informatiques distribués . . . . . . . . . . . . . . . . . . . . . . . . . . . 178 20.9 Groupes de Recherche et Développement . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 179 20.10 Formation des utilisateurs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180 20.11 Conduite de projets européens . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180 20.12 L’Euro-Interferometry Initiative . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 180 20.13 Darwin . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 182 20.14 Relations avec l’ESO et le MSC . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 182 20.15 Prospective . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 183 11
Page 3: LABORATOIRE D’ASTROPHYSIQUE DE GR
Page 6 and 7: III Team ASTROMOL 41 2 Presentation
Page 8 and 9: 8.1.3 Graduate Students . . . . . .
Page 13: Part I Foreword: Presentation of th
Page 17: Part II Executive Summary A 18th ce
Page 20 and 21: of CNRS for technicians and enginee
Page 22 and 23: Figure 1.3: New LAOG organigram (20
Page 24 and 25: 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
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Rate constant (cm 3 s -1 ) 1e-09 1e
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• One of us (PV) is strongly invo
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sublimation of water ice trapped ei
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If the chemistry in the first phase
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4.2.2 Molecular Physics The theoret
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Source Herschel Time Astromol Class
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several important studies that anti
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Chapter 5 Selected Publications •
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Part IV TEAM FOST The first image o
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393254 (5MJup at 55 AU) & AB Pic (1
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2.2 µ m 0.5" 11.7 µ m Figure 6.1:
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Figure 6.3: Contribution of heating
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such mid-term (several weeks) magne
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systems: HD 141569, HD 32297, HD 18
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C2D Spitzer/IRAC and MIPS data of s
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et al. 2002; 2003). We have found t
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Figure 6.8: Distribution of separat
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with only three known to date. Most
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300 objects, a size sufficient for
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therefore no surprise that vast eff
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data to verify the predictions we a
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Chapter 8 Appendices 8.1 Members of
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106
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108
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equipments for these tasks, from de
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10.1.3 Current trend of large equip
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• Improving High Angular Resoluti
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Chapter 11 Results 11.1 Towards hig
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Figure 11.2: NAOS-CONICA image of t
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on PUEO at CFHT. The IFS experts (A
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Figure 11.5: Image of the binary st
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Figure 11.7: PICNIC low noise infra
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have taken responsibilities: A. Che
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Figure 11.10: thermal modeling of W
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Figure 12.1: All the GRIL projects
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12.2 Optical interferometry As for
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the VLTI. CHARA is equipped with an
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• ANR Alterdetect, with IMEP : si
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Mixed GRIL-other team profiles 1. A
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Name Grade Comm. Project Berger Jea
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• First fringes in the H band wit
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144
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146
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Table 15.1: List of the permanent S
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15.4 Transport phenomena in accreti
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Figure 15.2: Spectral energy distri
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states, combining a still powerful
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Excitation of turbulence by Cosmic
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Table 15.2: Former PhD students of
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Chapter 16 Perspectives The distinc
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Ray background. The second project
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164
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- Ceccarelli Cecilia (AT) - Delfoss
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Among the various areas of expertis
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-responsable du groupe ”logiciel
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Chef de l’ Equipe ASTROMOL du LAO
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jury de concours: 1 concours IR CNR
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Chapter 20 Appendix 4: The Jean Mar
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20.7 Production informatique ¡¢£
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20.10 Formation des utilisateurs La
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20.13 Darwin ¡¢£¤¥¦§¨©�
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Untitled - Laboratoire d'Astrophysique de l'Observatoire de Grenoble

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