Trapping dust particles in the outer regions of protoplanetary disks

Astronomy and Astrophysics

Volumn 538, Issue , 2012, Pages

  Pinilla, P ^a,b   Birnstiel, T ^c,d   Ricci, L ^e,f   Dullemond, C P ^a,b   Uribe, A L ^b   Testi, L ^f,g   Natta, A ^g  

^a UNIVERSITY OF HEIDELBERG   (Germany)

^b MAX PLANCK INSTITUT FÜR ASTRONOMIE   (Germany)

^c UNIVERSITY OF MUNICH   (Germany)

^d EXCELLENCE CLUSTER UNIVERSE   (Germany)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^g INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

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

Indexed keywords

ACCRETION , ACCRETION DISKS; ANTENNA CONFIGURATIONS; BUMPY SURFACE; CIRCUMSTELLAR MATTERS; DIFFERENT FREQUENCY; DUST PARTICLE; GAS DENSITY; INHOMOGENEITIES; LARGE PARTICLES; LENGTH SCALE; MAGNETOROTATIONAL INSTABILITY; PRESSURE PROFILES; PROTOPLANETARY DISKS; RING STRUCTURES; SIMULATED IMAGES; SINUSOIDAL DISTURBANCES; SOFTWARE APPLICATIONS; SPECTRAL SLOPES; STAR-FORMING REGION; STARS: PRE-MAIN SEQUENCE; TIME-SCALES;

COMPUTER SOFTWARE; GRAIN GROWTH; SATELLITES;

STARS;

EID: 84856867784     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118204     Document Type: Article

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