286 citations · 1.4k across the 35 of their papers we have counts for
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Measuring the Dust Masses of Protoplanetary Disks in Lupus with ALMA: Evidence that Disks can be Optically Thick at 3 mm
Z. Xin, C. C. Espaillat, A. M. Rilinger +2
Accurate disk mass measurements are necessary to constrain disk evolution and the timescale of planet formation, but such measurements are difficult to make and are very dependent…
Determining Dust Properties in Protoplanetary Disks: SED-derived Masses and Settling With ALMA
Anneliese Rilinger, Catherine Espaillat, Zihua Xin +3
We present spectral energy distribution (SED) modeling of 338 disks around T Tauri stars from eleven star-forming regions, ranging from 0.5 to 10 Myr old. The disk masses we…
Gaia EDR3 comparative study of protoplanetary disk fractions in young stellar clusters
I. Mendigutía, E. Solano, M. Vioque +4
(Abridged) The lifetime of protoplanetary disks around young stars limits the timescale when planets form. A disk dissipation timescale < 10 Myr was inferred from surveys providing…
Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): A Panchromatic View of DO Tau's Complex Kilo-au Environment
Jane Huang, Christian Ginski, Myriam Benisty +20
While protoplanetary disks are often treated as isolated systems in planet formation models, observations increasingly suggest that vigorous interactions between Class II disks and…
A highly settled disk around Oph 163131
M. Villenave, K. R. Stapelfeldt, G. Duchene +10
High dust density in the midplane of protoplanetary disks is favorable for efficient grain growth and can allow fast formation of planetesimals and planets, before disks dissipate.…