Evidence for a hot dust-free inner disk around 51 Oph

Astronomy and Astrophysics

Volumn 430, Issue 3, 2005, Pages

  Thi, W F ^a   Van Dalen, B ^a   Bik, A ^a,b   Waters, L B F M ^a,c  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^c KU LEUVEN   (Belgium)

Author keywords

Accretion disks; Planetary systems: protoplanetary disks; Stars: formation

Indexed keywords

DATA REDUCTION; INFRARED RADIATION; INFRARED SPECTROMETERS; PHOTODISSOCIATION; PLANETS; SIGNAL TO NOISE RATIO; TRAJECTORIES;

DUST SUBLIMATION; PROTOPLANETARY DISKS; SPECTRAL ENERGY DISTRIBUTION (SED); STARS;

ASTROPHYSICS;

EID: 13444301233     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:200400132     Document Type: Article

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