530 citations · 1.5k across the 12 of their papers we have counts for
12 papers
Observational Completion Limit of Minor Planets from the Asteroid Belt to Jupiter Trojans
Nathanial P Hendler, Renu Malhotra
With the growing numbers of asteroids being discovered, identifying an observationally complete sample is essential for statistical analyses and for informing theoretical models of…
Hints for icy pebble migration feeding an oxygen-rich chemistry in the inner planet-forming region of disks
Andrea Banzatti, Ilaria Pascucci, Arthur D. Bosman +9
We present a synergic study of protoplanetary disks to investigate links between inner disk gas molecules and the large-scale migration of solid pebbles. The sample includes 63 dis…
Dual-Wavelength ALMA Observations of Dust Rings in Protoplanetary Disks
Feng Long, Paola Pinilla, Gregory J. Herczeg +13
We present new Atacama Large Millimeter/submillimeter Array (ALMA) observations for three protoplanetary disks in Taurus at 2.9\,mm and comparisons with previous 1.3\,mm data both…
The evolution of dust-disk sizes from a homogeneous analysis of 1-10 Myr-old stars
Nathanial Hendler, Ilaria Pascucci, Paola Pinilla +4
We utilize ALMA archival data to estimate the dust disk size of 152 protoplanetary disks in Lupus (1-3 Myr), Chamaeleon I (2-3 Myr), and Upper-Sco (5-11 Myr). We combine our sample…
Compact Disks in a High Resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud
Feng Long, Gregory J. Herczeg, Daniel Harsono +24
We present a high-resolution (, au, mean sensitivity of Jy~beam at 225 GHz) snapshot survey of 32 protoplanetary disks around young stars with spe…
The newborn planet population emerging from ring-like structures in discs
G. Lodato, G. Dipierro, E. Ragusa +23
ALMA has observed a plethora of ring-like structures in planet forming discs at distances of 10-100 au from their host star. Although several mechanisms have been invoked to explai…
The Ring Structure in the MWC 480 Disk Revealed by ALMA
Yao Liu, Giovanni Dipierro, Enrico Ragusa +20
Gap-like structures in protoplanetary disks are likely related to planet formation processes. In this paper, we present and analyze high resolution (0.17*0.11 arcsec) 1.3 mm ALMA c…
Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region
Feng Long, Paola Pinilla, Gregory J. Herczeg +23
Rings are the most frequently revealed substructure in ALMA dust observations of protoplanetary disks, but their origin is still hotly debated. In this paper, we identify dust subs…
An ALMA Survey of faint disks in the Chamaeleon I star-forming region: Why are some Class II disks so faint?
Feng Long, Gregory J. Herczeg, Ilaria Pascucci +6
ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate eit…
A likely planet-induced gap in the disk around T Cha
Nathanial P. Hendler, Paola Pinilla, Ilaria Pascucci +7
We present high resolution () 3mm ALMA observations of the highly inclined transition disk around the star T Cha. Our continuum image reveals multiple dust struct…
An ALMA Survey of CO isotopologue emission from Protoplanetary Disks in Chamaeleon I
Feng Long, Gregory J. Herczeg, Ilaria Pascucci +8
The mass of a protoplanetary disk limits the formation and future growth of any planet. Masses of protoplanetary disks are usually calculated from measurements of the dust continuu…
Hints for Small Disks around Very Low-Mass Stars and Brown Dwarfs
Nathanial Hendler, Gijs D. Mulders, Ilaria Pascucci +6
The properties of disks around brown dwarfs and very-low mass stars (hereafter VLMOs) provide important boundary conditions on the process of planet formation and inform us about t…