activity
20222024
most citedEarly Planet Formation in Embedded Disks (eDisk) IX: High-resolution ALMA Observations of the Class 0 Protostar R CrA IRS5N and its surrounding

17 citations · 25 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP20247 cited

Early Planet Formation in Embedded Disks (eDisk). XI. A high-resolution view toward the BHR 71 Class 0 protostellar wide binary

Sacha Gavino, Jes K. Jørgensen, Rajeeb Sharma +25

We present Atacama Large Millimeter/submillimeter Array (ALMA) observations of the binary Class 0 protostellar system BHR 71 IRS1 and IRS2 as part of the Early Planet Formation in…

astro-ph.EP20241 cited

Mind the Trap: Non-negligible effect of volatile trapping in ice on C/O ratios in protoplanetary disks and exoplanetary atmospheres

N. F. W. Ligterink, K. A. Kipfer, S. Gavino

The ability of bulk ices (HO, CO) to trap volatiles has been well studied in any experimental sense, but largely ignored in protoplanetary disk and planet formation mod…

astro-ph.EP2024

Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a

Shigehisa Takakuwa, Kazuya Saigo, Miyu Kido +22

We performed radiative transfer calculations and observing simulations to reproduce the 1.3-mm dust-continuum and CO (2-1) images in the Class I protostar R CrA IRS7B-a, obs…

astro-ph.EP202317 cited

Early Planet Formation in Embedded Disks (eDisk) IX: High-resolution ALMA Observations of the Class 0 Protostar R CrA IRS5N and its surrounding

Rajeeb Sharma, Jes K. Jørgensen, Sacha Gavino +19

We present high-resolution, high-sensitivity observations of the Class 0 protostar RCrA IRS5N as part of the Atacama Large Milimeter/submilimeter Array (ALMA) large program Early P…

astro-ph.SR2022

A VLA View of the Flared, Asymmetric Disk Around the Class 0 Protostar L1527 IRS

Patrick D. Sheehan, John J. Tobin, Zhi-Yun Li +21

We present high resolution Karl G. Jansky Very Large Array (VLA) observations of the protostar L1527 IRS at 7 mm, 1.3 cm, and 2 cm wavelengths. We detect the edge-on dust disk at a…