Sensitive limits on the abundance of cold water vapor in the DM Tauri protoplanetary disk

Astronomy and Astrophysics

Volumn 521, Issue 1, 2010, Pages

  Bergin, E A ^a   Hogerheijde, M R ^b   Brinch, C ^b   Fogel, J ^a   Yildiz, U A ^b   Kristensen, L E ^b   Van Dishoeck, E F ^b,c   Bell, T A ^d   Blake, G A ^e   Cernicharo, J ^f   Dominik, C ^f,g   Lis, D ^h   Melnick, G ⁱ   Neufeld, D ^j   Panic O ^k   Pearson, J C ^l   Bachiller, R ^m   Baudry, A ⁿ   Benedettini, M ^o   Benz, A O ^p   Bjerkeli, P ^q   Bontemps, S ^r,ak   Braine, J ^s   Bruderer, S ^p   Caselli, P ^o,s   Codella, C ^o   Daniel, F ^e   Di Giorgio, A M ⁿ   Doty, S D ^t   Encrenaz, P ^u   Fich, M ^v   Fuente, A ^m   Giannini, T ^w   Goicoechea, J R ^e   De Graauw, Th ^x   Helmich, F ^x   Herczeg, G J ^c   Herpin, F ⁿ   Jacq, T ^o   Johnstone, D ^y,z   Jorgensen J K ^aa   Larsson, B ^ab   Liseau, R ^q   Marseille, M ^x   Mc Coey, C ^v,ac   Nisini, B ⁿ   Olberg, M ^q   Parise, B ^ad   Plume, R ^ae   Risacher, C ^x   Santiago Garcia J ^af   Saraceno, P ⁿ   Shipman, R ^x   Tafalla, M ^m   Van Kempen, T A ⁱ   Visser, R ^b   Wampfler, S F ^p   Wyrowski, F ^ad   Van Der Tak, F ^x,ag   Jellema, W ^x   Tielens, A G G M ^b   Hartogh, P ^ah   Stutzki J ^ai   Szczerba, R ^aj   more..

^a UNIVERSITY OF MICHIGAN   (United States)

^b LEIDEN UNIVERSITY   (Netherlands)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e INSTITUTO NACIONAL DE TÉCNICA AEROESPACIAL   (Spain)

^f UNIVERSITY OF AMSTERDAM   (Netherlands)

^g RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^j JOHNS HOPKINS UNIVERSITY   (United States)

^k EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^l CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^m OBSERVATORIO ASTRONÓMICO NACIONAL   (Spain)

ⁿ INAF   (Italy)

^o INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^p ETH ZURICH   (Switzerland)

^q CHALMERS UNIVERSITY OF TECHNOLOGY   (Sweden)

^r UNIVERSITÉ DE BORDEAUX   (France)

^s UNIVERSITY OF LEEDS   (United Kingdom)

^t DENISON UNIVERSITY   (United States)

^u OBSERVATOIRE DE PARIS   (France)

^v UNIVERSITY OF WATERLOO   (Canada)

^w INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^x SRON NETHERLANDS INSTITUTE FOR SPACE RESEARCH   (Netherlands)

^y NATIONAL RESEARCH COUNCIL CANADA   (Canada)

^z UNIVERSITY OF VICTORIA   (Canada)

^aa UNIVERSITY OF COPENHAGEN   (Denmark)

^ab STOCKHOLM UNIVERSITY   (Sweden)

^ac UNIVERSITY OF WESTERN ONTARIO   (Canada)

^ad MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

^ae UNIVERSITY OF CALGARY   (Canada)

^af Institute de Radioastronomie Millimétrique IRAM Núcleo Central   (Spain)

^ag UNIVERSITY OF GRONINGEN   (Netherlands)

^ah MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^ai UNIVERSITY OF COLOGNE   (Germany)

^aj NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^ak LABORATOIRE D ASTROPHYSIQUE DE BORDEAUX   (France)

more..

Author keywords

ISM: abundances; ISM: molecules; protoplanetary disks

Indexed keywords

GROUND STATE;

EMISSION LINES; INTEGRATED INTENSITIES; ISM: ABUNDANCE; ISM: MOLECULES; LINE STRENGTH; MODEL CALCULATIONS; PROTOPLANETARY DISKS; WIDE-BAND;

WATER VAPOR;

EID: 77957669169     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015104     Document Type: Article

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