202 citations · 391 across the 12 of their papers we have counts for
14 papers
Measuring the and isotopic ratios of volatile sulfur during planet formation
Alice S. Booth, Maria N. Drozdovskaya, Milou Temmink +9
Stable isotopic ratios constitute powerful tools for unraveling the thermal and irradiation history of volatiles. In particular, we can use our knowledge of the isotopic fractionat…
Rocky planet formation in compact disks around M dwarfs
M. Sanchez, N. van der Marel, M. Lambrechts +2
Rocky planets in compact configurations are the most common ones around M dwarfs. Many disks around very low mass stars (between 0.1 and 0.5 M) are rather compact and small…
An ALMA molecular inventory of warm Herbig Ae disks: II. Abundant complex organics and volatile sulphur in the IRS 48 disk
Alice S. Booth, Milou Temmink, Ewine F. van Dishoeck +11
The Atacama Large Millimeter/submillimeter Array (ALMA) can probe the molecular content of planet-forming disks with unprecedented sensitivity. These observations allow us to build…
An ALMA molecular inventory of warm Herbig Ae disks: I. Molecular rings, asymmetries and complexity in the HD 100546 disk
Alice S. Booth, Margot Leemker, Ewine F. van Dishoeck +11
Observations of disks with the Atacama Large Millimeter/submillimeter Array (ALMA) allow us to map the chemical makeup of nearby protoplanetary disks with unprecedented spatial res…
Correlation between accretion rate and free-free emission in protoplanetary disks -- A multi-wavelength analysis of central mm/cm emission in transition disks
Alessia A. Rota, Jurrian D. Meijerhof, Nienke van der Marel +3
The inner regions of protoplanetary disks are the locations where most of planets are thought to form and where processes that influence the global evolution of the disk, such as M…
Finding substructures in protostellar disks in Ophiuchus
Arnaud Michel, Sarah I. Sadavoy, Patrick D. Sheehan +5
High-resolution, millimeter observations of disks at the protoplanetary stage reveal substructures such as gaps, rings, arcs, spirals, and cavities. While many protoplanetary disks…