12 citations · 14 across the 4 of their papers we have counts for
4 papers
MINDS: Detection of an inner gas disk caused by evaporating bodies around HD 172555
M. Samland, T. Henning, A. Caratti o Garatti +23
Mechanisms such as collisions of rocky bodies or cometary activity give rise to dusty debris disks. Debris disks trace the leftover building blocks of planets, and thus also planet…
On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres
Adina D. Feinstein, Richard A. Booth, Jennifer B. Bergner +34
Measuring a single elemental ratio (e.g., carbon-to-oxygen) provides insufficient information for understanding the formation mechanisms and evolution that affect our observations…
Variations of the HCO, HCN, HNC, NH and NH deuterium fractionation in high-mass star-forming regions
A. G. Pazukhin, I. I. Zinchenko, E. A. Trofimova +2
We use spectra and maps of the and DCO, DCN, DNC, lines and ortho- and para-NHD lines, obtained with the IRAM-30m telescope…
Chemistry in Protoplanetary Disks
Dmitry Semenov
Protoplanetary disks (PPDs) surrounding young stars are short-lived (~0.3-10 Myr), compact (~10-1000 AU) rotating reservoirs of gas and dust. PPDs are believed to be birthplaces of…