activity
20162019
most citedOne Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

205 citations · 509 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2019205 cited

One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Zhaohuan Zhu, Shangjia Zhang, Yan-Fei Jiang +10

ALMA surveys have suggested that the dust in Class II disks may not be enough to explain the averaged solid mass in exoplanets, under the assumption that the mm disk continuum emis…

astro-ph.SR2018153 cited

CO and dust properties in the TW Hya disk from high-resolution ALMA observations

Jane Huang, Sean M. Andrews, L. Ilsedore Cleeves +10

We analyze high angular resolution ALMA observations of the TW Hya disk to place constraints on the CO and dust properties. We present new, sensitive observations of the CO…

astro-ph.SR201797 cited

An ALMA survey of DCN/HCN and DCO/HCO in protoplanetary disks

Jane Huang, Karin I. Oberg, Chunhua Qi +7

The deuterium enrichment of molecules is sensitive to their formation environment. Constraining patterns of deuterium chemistry in protoplanetary disks is therefore useful for prob…

astro-ph.GA201754 cited

Nitrogen Fractionation in Protoplanetary Disks from the H13CN/HC15N Ratio

V. V. Guzmán, K. I. Öberg, J. Huang +2

Nitrogen fractionation is commonly used to assess the thermal history of Solar System volatiles. With ALMA it is for the first time possible to directly measure 14N/15N ratios in c…

astro-ph.SR2016

Evidence for a CO desorption front in the outer AS 209 disk

Jane Huang, Karin I. Oberg, Sean M. Andrews

Millimeter observations of CO isotopologues are often used to make inferences about protoplanetary disk gas density and temperature structures. The accuracy of these estimates depe…

astro-ph.GA2016

Constraining the size of the carrier of the 5797.1 diffuse interstellar band

Jane Huang, Takeshi Oka

The diffuse interstellar band (DIB) at 5797.1 Å is simulated based on three premises: (1) The carrier of the DIB is polar as concluded by T. Oka et al. from the anomalous spectrum…