Testing the theory of grain growth and fragmentation by millimeter observations of protoplanetary disks

Astronomy and Astrophysics

Volumn 516, Issue 25, 2010, Pages

  Birnstiel, T ^a   Ricci, L ^b   Trotta, F ^b,c   Dullemond, C P ^a   Natta, A ^c   Testi, L ^b,c   Dominik, C ^d,e   Henning, T ^a   Ormel, C W ^a   Zsom, A ^a  

^a MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^d UNIVERSITY OF AMSTERDAM   (Netherlands)

^e RADBOUD UNIVERSITY NIJMEGEN   (Netherlands)

Author keywords

accretion, accretion disks; circumstellar matter; planets and satellites: formation; protoplanetary disks; stars: pre main sequence; submillimeter: stars

Indexed keywords

DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); DUST; GRAIN SIZE AND SHAPE; MODELS; PLANETS; SATELLITES; STARS;

ACCRETION , ACCRETION DISKS; CIRCUMSTELLAR MATTERS; PLANETS AND SATELLITES: FORMATION; PROTOPLANETARY DISKS; STARS: PRE-MAIN-SEQUENCE; SUBMILLIMETER: STARS;

GRAIN GROWTH;

EID: 77957582719     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014893     Document Type: Article

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