Transition disks: Four candidates for ongoing giant planet formation in Ophiuchus

Astronomy and Astrophysics

Volumn 539, Issue , 2012, Pages

  Orellana, M ^a,b   Cieza, L A ^c   Schreiber, M R ^b   Merin B ^d   Brown, J M ^e   Pellizza, L J ^a,f   Romero, G A ^b  

^a Universidad Nacional de Río Cuarto Consejo Nacional de Investigaciones Científicas y Técnicas   (Argentina)

^b UNIVERSIDAD DE VALPARAÍSO   (Chile)

^c UNIVERSITY OF HAWAII   (United States)

^d EUROPEAN SPACE AGENCY   (Spain)

^e HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^f INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

Author keywords

protoplanetary disks; stars: pre main sequence; submillimeter: planetary systems

Indexed keywords

BEST-FIT MODEL PARAMETERS; DENSITY PROFILE; DUST DISTRIBUTION; DUST SETTLING; GIANT PLANET FORMATION; GIANT PLANETS; INNER CAVITIES; MONTE CARLO; MONTE CARLO MARKOV CHAIN; PARAMETER SPACES; PARAMETER VALUES; PARAMETRIC MODELS; PROTOPLANETARY DISKS; SPECTRAL ENERGY DISTRIBUTION; STARS: PRE-MAIN SEQUENCE; STATISTICAL CONFIDENCE; SUBMILLIMETER: PLANETARY SYSTEMS; TEMPERATURE STRUCTURE; THERMAL EQUILIBRIUMS;

GRAIN GROWTH; STARS;

DUST;

EID: 84863116436     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201117659     Document Type: Article

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