papers

Publications (33)

astro-ph.SR2025

HDO ice detected toward an isolated low-mass protostar with JWST

Katerina Slavicinska, Łukasz Tychoniec, María Gabriela Navarro +15

Water is detected in environments representing every stage of star and solar system formation, but its chemical evolution throughout these stages remains poorly constrained. Deuter…

astro-ph.EP2023

Early Planet Formation in Embedded Disks (eDisk). II. Limited Dust Settling and Prominent Snow Surfaces in the Edge-on Class I Disk IRAS 04302+2247

Zhe-Yu Daniel Lin, Zhi-Yun Li, John J. Tobin +26

While dust disks around optically visible, Class II protostars are found to be vertically thin, when and how dust settles to the midplane are unclear. As part of the Atacama Large…

astro-ph.SR2018

Multiple Gaps in the Disk of the Class I Protostar GY 91

Patrick Sheehan, Josh Eisner

We present the highest spatial resolution ALMA observations to date of the Class I protostar GY 91 in the Ophiuchus L1688 molecular cloud complex. Our 870 m and 3 mm dust…

astro-ph.SR2017

Improved Constraints on the Disk Around MWC 349A from the 23-Meter LBTI

Steph Sallum, Josh Eisner, Phil Hinz +4

We present new spatially resolved observations of MWC 349A from the Large Binocular Telescope Interferometer (LBTI), a 23-meter baseline interferometer made up of two, co-mounted 8…

astro-ph.SR2014

Constraining the Disk Masses of the Class I Binary Protostar GV Tau

Patrick Sheehan, Josh Eisner

We present new spatially resolved 1.3 mm imaging with CARMA of the GV Tau system. GV Tau is a Class I binary protostar system in the Taurus Molecular Cloud, the components of which…

astro-ph.GA2021

Detection of Substructures in Young Transition Disk WL 17

Hannah Gulick, Sarah Sadavoy, Luca Matra +2

WL 17 is a young transition disk in the Ophiuchus L1688 molecular cloud complex. Even though WL 17 is among the brightest disks in L1688 and massive enough to expect dust self-scat…