Consistent dust and gas models for protoplanetary disks I. Disk shape, dust settling, opacities, and PAHs (2016)
Attributed to:
Astrophysics at St Andrews: 2012-2014
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201526538
Publication URI: http://dx.doi.org/10.1051/0004-6361/201526538
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics