activity
20152022
most citedDestruction of Refractory Carbon in Protoplanetary Disks

69 citations · 176 across the 5 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

6 papers · 1 filter

astro-ph.EP202231 cited

New Constraints on Protoplanetary Disk Gas Masses in Lupus

Dana E. Anderson, L. Ilsedore Cleeves, Geoffrey A. Blake +4

Gas mass is a fundamental quantity of protoplanetary disks that directly relates to their ability to form planets. Because we are unable to observe the bulk H content of disks…

astro-ph.EP2021

Simulating Observations of Ices in Protoplanetary Disks

Nicholas P. Ballering, L. Ilsedore Cleeves, Dana E. Anderson

Ices are an important constituent of protoplanetary disks. New observational facilities, notably the James Webb Space Telescope (JWST), will greatly enhance our view of disk ices b…

astro-ph.EP202145 cited

Observing Carbon & Oxygen Carriers in Protoplanetary Disks at Mid-infrared Wavelengths

D. E. Anderson, G. A. Blake, L. I. Cleeves +5

Infrared observations probe the warm gas in the inner regions of planet-forming disks around young sun-like, T Tauri stars. In these systems, HO, OH, CO, CO, CH, an…

astro-ph.EP201931 cited

Unlocking CO Depletion in Protoplanetary Disks II. Primordial C/H Predictions Inside the CO Snowline

Kamber R. Schwarz, Edwin A. Bergin, L. Ilsedore Cleeves +4

CO is thought to be the main reservoir of volatile carbon in protoplanetary disks, and thus the primary initial source of carbon in the atmospheres of forming giant planets. Howeve…

astro-ph.EP2018

Unlocking CO Depletion in Protoplanetary Disks I. The Warm Molecular Layer

Kamber R. Schwarz, Edwin A. Bergin, L. Ilsedore Cleeves +4

CO is commonly used as a tracer of the total gas mass in both the interstellar medium and in protoplanetary disks. Recently there has been much debate about the utility of CO as a…

astro-ph.EP201769 cited

Destruction of Refractory Carbon in Protoplanetary Disks

Dana E. Anderson, Edwin A. Bergin, Geoffrey A. Blake +3

The Earth and other rocky bodies in the inner solar system contain significantly less carbon than the primordial materials that seeded their formation. These carbon-poor objects in…