activity
20242026
most citedDiscovery of carbon monoxide emission from five debris disks around young A-type stars

2 citations · 2 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2026

Peering into the Midplane of the DM Tau Disk using N2H+ and DCO+

Amina Diop, Kevin Flaherty, Chunhua Qi +7

Planets form in the midplanes of protoplanetary disks, thus investigating the properties of the midplane region can shed light on the physical and chemical processes governing the…

astro-ph.SR2026

Mapping Molecular Ion Distributions in a Diverse Sample of Protoplanetary Disks

Deryl E. Long, L. Ilsedore Cleeves, Charles J. Law +10

Observations of ionization-tracing molecules in protoplanetary disks suggest that their ionization environments are diverse due to varying degrees of cosmic ray modulation, stellar…

astro-ph.GA2026

Spatially-resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA2

L. Pantoni, F. Galliano, S. C. Madden +62

Large dust grains in thermal equilibrium dominate the far-infrared and contribute to the millimetre continuum of star-forming galaxies, but constraining their properties is difficu…

astro-ph.EP2025★ 2 cited

Discovery of carbon monoxide emission from five debris disks around young A-type stars

A. Moór, P. Ábrahám, Á +7

Over the past fifteen years, surveys mainly at millimeter wavelengths have led to the discovery of 20 gas-bearing debris disks, most of them surrounding young intermediate-ma…

astro-ph.SR2024

Exploring the Complex Ionization Environment of the Turbulent DM Tau Disk

Deryl E. Long, L. Ilsedore Cleeves, Fred C. Adams +9

Ionization drives important chemical and dynamical processes within protoplanetary disks, including the formation of organics and water in the cold midplane and the transportation…

astro-ph.EP2024

Low CI/CO Abundance Ratio Revealed by HST UV Spectroscopy of CO-rich Debris Disks

Aoife Brennan, Luca Matrà, Sebastián Marino +6

The origin and evolution of CO gas in debris disks has been debated since its initial detection. The gas could have a primordial origin, as a remnant of the protoplanetary disk or…