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

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III Team ASTROMOL 41 2 Presentation and Scientific Objectives 43 2.1 Presentation of Astromol: composition, goals and summary of activities . . . . . . . . . . . . . . 43 2.2 Observations at the telescopes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 45 2.3 Development of astrophysical models . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46 2.4 Molecular physics: theories and codes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 46 2.5 Publications . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 2.6 Teaching and students formation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 2.7 National and international collaborations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 47 3 Results 49 3.1 Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49 3.2 Star Formation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50 3.2.1 Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50 3.2.2 The deuteration in the first phases of star formation . . . . . . . . . . . . . . . . . . . . . 50 3.2.3 The hot corinos of solar type protostars . . . . . . . . . . . . . . . . . . . . . . . . . . . . 51 3.2.4 The outflows of protostars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53 3.2.5 The intermediate/high mass protostars . . . . . . . . . . . . . . . . . . . . . . . . . . . . 53 3.2.6 The X-rays from young protostars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 54 3.2.7 Dust around protostars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 3.3 Molecular Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 3.3.1 Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 56 3.3.2 Potential energy surfaces . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 57 3.3.3 Energy transfer processes . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58 3.4 High Performance Computing . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 61 3.5 Proto-planetary Disks: where Astromol meets FOST . . . . . . . . . . . . . . . . . . . . . . . . . 62 4 Perspectives 65 4.1 Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65 4.2 Scientific goals . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 65 4.2.1 Star Formation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 66 4.2.2 Molecular Physics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 68 4.3 The involvement in the large international projects: Herschel and ALMA . . . . . . . . . . . . . 69 6
4.4 The European Network “The Molecular Universe” . . . . . . . . . . . . . . . . . . . . . . . . . . 70 4.5 Cosmology: a new frontier for Astromol ? . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 71 4.6 The needs of Astromol : accretion and recruitment . . . . . . . . . . . . . . . . . . . . . . . . . . 72 5 Selected Publications 74 IV Team FOST 77 6 Introduction of the team & Science Results 79 6.1 FOST: a short presentation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79 6.2 Scientific Highlights . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 79 6.3 Selected topics in Star Formation . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 80 6.3.1 Young Accretion Disks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81 6.3.2 The star-disk interaction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 85 6.3.3 Physics of Jets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 87 6.3.4 Observations of Debris disks . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 87 6.3.5 Dynamical Models . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88 6.3.6 Other topics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 88 6.4 Selected topics on the IMF and the properties of low-mass populations . . . . . . . . . . . . . . . 90 6.4.1 Nearby Star Forming Regions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 90 6.4.2 Selected Intermediate Age Clusters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 92 6.4.3 The Solar Neighbourhood . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 93 6.5 Selected topics on Extra-Solar Planets . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 96 6.5.1 Exoplanets around M Dwarfs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 97 6.5.2 Exoplanets around F- and A-stars . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 98 6.5.3 Exoplanets in Nearby associations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 7 Future Research Directions 101 7.1 Research Plans . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 101 7.2 Needs in personnel . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 102 8 Appendices 104 8.1 Staff . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104 8.1.1 permanent staff . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104 8.1.2 Post-docs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 104 7
Page 3: LABORATOIRE D’ASTROPHYSIQUE DE GR
Page 8 and 9: 8.1.3 Graduate Students . . . . . .
Page 10 and 11: VI Team SHERPA 145 15 Results 147 1
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
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tens of visual magnitudes, hence pr
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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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