[tel-00726959, v1] CaractÃ©riser le milieu interstellaire ... - HAL - INRIA

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H. S. Liszt and J. Pety: Imaging diffuse clouds: bright and dark gas mapped in CO50˚B0954+6584110˚B1730-1302040135Galactic Latitude40˚30˚20Galactic Latitude0˚608010020204020˚40-60 -40 -20 0 20V LSR (KM S -1 )0-10˚0 50V LSR (KM S -1 )0tel-00726959, version 1 - 31 Aug 2012Galactic Latitude20˚10˚0˚40206020 4060 801000 50V LSR (KM S -1 )2060 40 80100135B1928+738 B1954+513200119Galactic Latitude10˚0˚-10˚-20˚40806020 40 60-100 -50 0V LSR (KM S -1 )B2251+15820801180300˚Galactic Latitude-10˚B2200+42020Galactic Latitude-30˚-40˚-50˚2040-60˚-100 -50 0V LSR (KM S -1 )00-60 -40 -20 0 20V LSR (KM S -1 )Fig. B.2. Latitude-velocity diagrams of H I brightness around six background targets used for mm-wave molecular absorption studies, usingH I data from the LDSS survey (Hartmann & Burton 1997), as in Fig. B.1.A58, page 23 of 23
tel-00726959, version 1 - 31 Aug 2012Chapitre 5Copyright: CFHT/CoelumLa Tête de Cheval : une référence observationnellepour les modèles chimiques5.1 Les modèles photochimiques et la Tête de ChevalLes modèles des régions de photo-dissociations (PDRs) sont utilisés pour comprendre l’évolutionde la matière éclairée par le rayonnement UV, à la fois dans notre galaxie et dans lesgalaxies extérieures. Au vu de la complexité inhérente à la constitution de réseaux et de modèleschimiques fiables, il y a un vrai besoin d’observations bien contraintes qui puissent servir de
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UNIVERSITÉ PIERRE ET MARIE CURIEHA
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Table des matières1 Rapport de sou
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Rapport après soutenanceHabilitati
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Chapitre 2Curriculum vitaetel-00726
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2.7 ANIMATION ET DIFFUSION DE LA CU
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2.8 PARCOURS 131992-1993 ÉCOLE NOR
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Chapitre 3Copyright: IRAM/PdBIIntro
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Page 19 and 20: 4.2 ETUDES DIRECTES EN ÉMISSION 19
Page 21 and 22: 4.4 LA LUMINOSITY CO PAR MOLÉCULE
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Page 39 and 40: A&A 518, A45 (2010)If X HCO + is as
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A&A 494, 977-985 (2009)DOI: 10.1051
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M. Gerin et al.: HCO mapping of the
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Table 1. Observation parameters for
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7.2 MODE INTERFÉROMÉTRIQUE 161tel
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7.3 LE FUTUR DE LA RADIO-ASTRONOMIE
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CLASS evolution: I. Improved OTF su
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CLASS evolution: I. Improved OTF su
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A&A 526, A47 (2011)DOI: 10.1051/000
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S. Maret et al.: Weeds: a CLASS ext
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S. Maret et al.: Weeds: a CLASS ext
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IRAM-30m EMIR time/sensitivity esti
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IRAM-30m EMIR time/sensitivity esti
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Table C.1. Definition of the symbol
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IRAM Memo 2011-2WIFISYN:The GILDAS
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WIFISYN3. practiceWIFISYN3. practic
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WIFISYNA. implementation planWIFISY
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8.3 PERSPECTIVES 227tel-00726959, v
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3 REQUIREMENTS 44 CHANGES FOR END-U
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5 CHANGES FOR PROGRAMMERS 125 CHANG
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A EXHAUSTIVE DESCRIPTION OF THE CHA
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Chapitre 9Copyright: Stéphane Guis
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9.3 ACTIVITÉS 2008-2011 237tel-007
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Contribution de l'Action Spécique
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A. des multi-pixels à bure : une s
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5. besoins en services annexes, bé
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Articles publiés dans des revues
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ARTICLES PUBLIÉS DANS DES REVUES
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Mémos IRAM et ALMAtel-00726959, ve
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Actes de colloques nationaux et int
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ACTES DE COLLOQUES NATIONAUX ET INT
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