Dust properties of protoplanetary disks in the Taurus-Auriga star forming region from millimeter wavelengths

Astronomy and Astrophysics

Volumn 512, Issue 3, 2010, Pages

  Ricci, L ^a   Testi, L ^a,b   Natta, A ^b   Neri, R ^c   Cabrit, S ^d   Herczeg, G J ^e  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^c IRAM   (France)

^d OBSERVATOIRE DE PARIS   (France)

^e MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

Author keywords

Planets and satellites: formation; Protoplanetary disks; Stars: pre main sequence

Indexed keywords

COAGULATION; DISKS (MACHINE COMPONENTS); DUST; GRAIN GROWTH; GRAIN SIZE AND SHAPE; OPACITY; PLANETS; SATELLITES; SPECTROSCOPY; STARS;

ACCRETION RATE; ANALYSIS METHOD; AT-WAVELENGTH; CLASS II; DISK MODEL; DUST GRAINS; DUST MODELS; DUST OPACITY; DUST PARTICLE; EVOLUTIONARY STAGE; FAST PROCESS; HIGH DETECTION RATE; LARGE-GRAIN; MILLIMETER WAVELENGTH; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; SPATIAL EXTENSION; SPATIALLY RESOLVED; SPECTRAL ENERGY DISTRIBUTION; SPECTRAL INDICES; STAR-FORMING REGION; STARS: PRE-MAIN SEQUENCE; SUBMILLIMETERS; T TAURI STARS; TWO LAYERS; YOUNG STELLAR OBJECTS;

DISKS (STRUCTURAL COMPONENTS);

EID: 77953009390     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913403     Document Type: Article

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