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

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Ray background. The second project is VITRUV, a second generation VLTI instrument for aperture synthesis imaging with eight telescopes (PI: F. Malbet from LAOG). VITRUV will permit to obtain completely new results in a large numbers of astrophysical domains and in particular compact objects. Both projects are in a R&D level and we (mainly P.O. Petrucci and G. Henri) participate, since the beginning, to the scientific specification of both instruments. Other new <strong>de</strong>velopments will come from the contact with all the astroparticle facilities such as Pierre Auger Observatory, Neutrino Observatory (NET Cube), Gravitational Wave Observatories (VIRGO, LISA). Within 10 to 15 years, we can reasonably expect that fascinating astrophysics <strong>de</strong>velopments will stem from correlating gamma-rays, neutrino and gravitational bursts from Black Hole environments. The AGNs containing double quasars are the most promising sources of gravitational waves for LISA. 162
Part VII APPENDICES 163
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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
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Figure 1.6: PhD student repartition
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• LAOG researchers (and publishin
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and published 95 papers in four yea
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• National astronomy programs. 4
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1.5 From dreams to reality: Human r
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and accretion disks with heavy nume
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emphasis on the chemistry of planet
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Part III TEAM ASTROMOL Sub-arcsecon
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• we develop quantum and classica
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Table shows not only the volume of
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• Herschel-HIFI: Astromol is invo
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particular, we calculated a 9D H2O-
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• The hot corinos. More spectacul
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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
Page 112 and 113: 10.1.3 Current trend of large equip
Page 114 and 115: • Improving High Angular Resoluti
Page 116 and 117: Chapter 11 Results 11.1 Towards hig
Page 118 and 119: Figure 11.2: NAOS-CONICA image of t
Page 120 and 121: on PUEO at CFHT. The IFS experts (A
Page 122 and 123: Figure 11.5: Image of the binary st
Page 124 and 125: Figure 11.7: PICNIC low noise infra
Page 126 and 127: have taken responsibilities: A. Che
Page 128 and 129: Figure 11.10: thermal modeling of W
Page 130 and 131: Figure 12.1: All the GRIL projects
Page 132 and 133: 12.2 Optical interferometry As for
Page 134 and 135: the VLTI. CHARA is equipped with an
Page 136 and 137: • ANR Alterdetect, with IMEP : si
Page 138 and 139: Mixed GRIL-other team profiles 1. A
Page 140 and 141: Name Grade Comm. Project Berger Jea
Page 142 and 143: • First fringes in the H band wit
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Page 148 and 149: Table 15.1: List of the permanent S
Page 150 and 151: 15.4 Transport phenomena in accreti
Page 152 and 153: Figure 15.2: Spectral energy distri
Page 154 and 155: states, combining a still powerful
Page 156 and 157: Excitation of turbulence by Cosmic
Page 158 and 159: Table 15.2: Former PhD students of
Page 160 and 161: Chapter 16 Perspectives The distinc
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Page 166 and 167: - Ceccarelli Cecilia (AT) - Delfoss
Page 168 and 169: Among the various areas of expertis
Page 170 and 171: -responsable du groupe ”logiciel
Page 172 and 173: Chef de l’ Equipe ASTROMOL du LAO
Page 174 and 175: jury de concours: 1 concours IR CNR
Page 176 and 177: Chapter 20 Appendix 4: The Jean Mar
Page 178 and 179: 20.7 Production informatique ¡¢£
Page 180 and 181: 20.10 Formation des utilisateurs La
Page 182 and 183: 20.13 Darwin ¡¢£¤¥¦§¨©�
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