2011/10/10 by D. M. Salter, M. R. Hogerheijde, R. F. J. van der Burg +2 · 2 citations
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics and Star Formation Studies #Circumstellar dust #Cosmic dust #Infrared #Millimeter #Population #Protoplanetary disk #Settling #Silicate #Stars #Stellar, planetary, and galactic studies #T Tauri star #astro-ph.GA
paper · pdf · doi:10.1051/0004-6361/201015411
Accepted for publication in A&A, 19 pages, 13 figures
openalex publication_date 2011/10/10 · arxiv created 2011/10/20 · arxiv updated 2015/05/29 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
Context. The gas and dust content of protoplanetary disks evolves over the course of a few Myr. As the stellar X-ray and UV light penetration of the disk depends sensitively on the dust properties, trace molecular species like HCO+, HCN, and CN are expected to show marked differences from photoprocessing effects as the dust content in the disk evolves.