activity
20132026
most citedThe VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. A Statistical Characterization of Class 0 and I Protostellar Disks

332 citations · 784 across the 36 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

23 papers · 1 filter

astro-ph.SR2026

Early Planet Formation in Embedded Disks (eDisk). XXIV: Systematic Investigation of Disk Structures based on Visibility Analysis

Mayank Narang, Jerry Xu, Leslie W. Looney +11

The dust continuum emission from young protostellar disks encodes key information about their mass distribution and early evolution, yet uniform high-resolution comparative studies…

astro-ph.SR2026

Nascent Embedded-protostar Survey in Taurus (NEST) I: Protostellar Multiplicity

Aislinn C. Plante, John J. Tobin, Patrick D. Sheehan +5

We present new ALMA 0.9 mm and VLA 9 mm observations in the Taurus Molecular Cloud (TMC) of 25 protostellar systems, containing 40 protostars, observed at 0.3" (~20 au) resolution.…

astro-ph.SR2026

Nascent Embedded-protostar Survey in Taurus (NEST) II: Measuring Dust Mass, Disk Size, and Gas Mass

Noshin Yesmin, Patrick Sheehan, John Tobin +6

Envelope-embedded protostellar disks represent the earliest stage of protoplanetary disk evolution, but their masses and sizes are difficult to measure because disk emission is ent…

astro-ph.SR2026

Protostellar Outflows Shed Light on the Dominant Close Companion Star Formation Pathways

Ryan Sponzilli, Leslie Looney, John J. Tobin +11

Understanding the formation pathway for close-companion protostars is central to unraveling the processes that govern stellar multiplicity and very early star formation. We analyze…

astro-ph.SR2025

A Bridge between Young Stars Formed by Gravitational Interaction

Youngwoo Choi, Woojin Kwon, Leslie W. Looney +1

The majority of stars are born in clustered environments. In these environments, close encounters between young stars with planet-forming disks are expected to occur frequently. Ho…

astro-ph.SR2025

Multi-band ALMA Polarization Observations of BHB07-11 Reveal Aligned Dust Grains in Complex Spiral Arm Structures

Austen Fourkas, Leslie W. Looney, Zhe-Yu Daniel Lin +8

Polarization-mode observations from the Atacama Large Millimeter/submillimeter Array (ALMA) are powerful tools for studying the dust grain populations in circumstellar disks. Many…

astro-ph.SR2025

The Hourglass-shaped Magnetic Fields and Dust Filaments in the HH 211 Protostellar Envelope

Youngwoo Choi, Woojin Kwon, Leslie W. Looney +4

Magnetic fields influence the structure and evolution of protostellar systems, thus understanding their role is essential for probing the earliest stages of star formation. We pres…

astro-ph.SR2025

Early Planet Formation in Embedded Disks (eDisk) XXII: Keplerian disk, disk structures and jets/outflows in the Class 0 protostar IRAS 04166+2706

Nguyen Thi Phuong, Chang Won Lee, John J. Tobin +20

We present ALMA observations of the Class 0 protostar IRAS 04166+2706, obtained as part of the ALMA large program Early Planet Formation in Embedded Disks (eDisk). These observatio…

astro-ph.SR2025

L1448 IRS3B: Dust Polarization Aligned with Spiral Features, Tracing Gas Flows

Leslie W. Looney, Zhe-Yu Daniel Lin, Zhi-Yun Li +11

Circumstellar disk dust polarization in the (sub)millimeter is, for the most part, not from dust grain alignment with magnetic fields but rather indicative of a combination of dust…

astro-ph.SR2025

Sub-Millimeter Variability in the Envelope & Warped Protostellar Disk of the Class 0 Protostar HOPS 358

Patrick D. Sheehan, Doug Johnstone, Carlos Contreras Peña +7

The JCMT Transient Survey recently discovered that the Class 0 protostar HOPS 358 decreased in 350 GHz continuum brightness by % over the course of four years before bright…

astro-ph.SR2025

An embedded Disk (eDisk) in the IceAge: Investigating the jet and outflow from CED 110 IRS4

Mayank Narang, Nagayoshi Ohashi, John J. Tobin +3

We present a comprehensive study of the large-scale structure, jet and outflow morphology, and kinematics of the Class 0/I protostellar binary Ced 110 IRS4, using JWST NIRCam (F150…

astro-ph.SR2025

Early Grain Growth in the Young Protostellar Disk HH 212 Supported by Dust Self-Scattering Modeling

Ying-Chi Hu, Chin-Fei Lee, Zhe-Yu Daniel Lin +3

Grain growth in disks around young stars plays a crucial role in the formation of planets. Early grain growth has been suggested in the HH 212 protostellar disk by previous polariz…

astro-ph.SR2024

JWST-IPA: Chemical Inventory and Spatial Mapping of Ices in the Protostar HOPS370 -- Evidence for an Opacity Hole and Thermal Processing of Ices

Himanshu Tyagi, Manoj P., Mayank Narang +35

The composition of protoplanetary disks, and hence the initial conditions of planet formation, may be strongly influenced by the infall and thermal processing of material during th…

astro-ph.SR2024★ 12 cited

Early Planet Formation in Embedded Disks (eDisk) XVI: An asymmetric dust disk driving a multi-component molecular outflow in the young Class 0 protostar GSS30 IRS3

Alejandro Santamaria-Miranda, Itziar de Gregorio-Monsalvo, Nagayoshi Ohashi +17

We present the results of the ALMA Large Program Early Planet Formation in Embedded disks observations of the Class 0 protostar GSS30 IRS3. Our observations included 1.3 mm continu…

astro-ph.SR2024

Early Planet Formation in Embedded Disks (eDisk) XV: Influence of Magnetic Field Morphology in Dense Cores on Sizes of Protostellar Disks

Hsi-Wei Yen, Jonathan P. Williams, Jinshi Sai +15

The magnetic field of a molecular cloud core may play a role in the formation of circumstellar disks in the core. We present magnetic field morphologies in protostellar cores of 16…

astro-ph.SR2024★ 1 cited

An Observational View of Structure in Protostellar Systems

John J. Tobin, Patrick D. Sheehan

The envelopes and disks that surround protostars reflect the initial conditions of star and planet formation and govern the assembly of stellar masses. Characterizing these structu…

astro-ph.SR2024

Early Planet Formation in Embedded Disks (eDisk) XIII: Aligned Disks with Non-Settled Dust Around the Newly Resolved Class 0 Protobinary R CrA IRAS 32

Frankie J. Encalada, Leslie W. Looney, Shigehisa Takakuwa +19

Young protostellar binary systems, with expected ages less than 10 years, are little modified since birth, providing key clues to binary formation and evolution. We prese…

astro-ph.SR2023

The Disk Orientations of Perseus Protostellar Multiples at 8 au Resolution

Nickalas K. Reynolds, John J. Tobin, Patrick D. Sheehan +6

We present a statistical characterization of circumstellar disk orientations toward 12 protostellar multiple systems in the Perseus molecular cloud using the Atacama Large Millimet…

astro-ph.SR2020★ 84 cited

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. III. Substructures in Protostellar Disks

Patrick D. Sheehan, John J. Tobin, Sam Federman +2

The prevalence of substructures in Myr old protoplanetary disks, which are often linked to planet formation, has raised the question of how early such features form, and…

astro-ph.SR2019★ 33 cited

The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars I. Identifying and Characterizing the Protostellar Content of the OMC2-FIR4 and OMC2-FIR3 Regions

John J. Tobin, S. Thomas Megeath, Merel van 't Hoff +31

We present ALMA (0.87~mm) and VLA (9~mm) observations toward OMC2-FIR4 and OMC2-FIR3 within the Orion integral-shaped filament that are thought to be the nearest regions of interme…

astro-ph.SR2019★ 18 cited

VLA cm-wave survey of young stellar objects in the Oph A cluster: constraining extreme UV- and X-ray-driven disk photo-evaporation -- A pathfinder for Square Kilometre Array studies

A. Coutens, H. B. Liu, I. Jiménez-Serra +28

Observations of young stellar objects (YSOs) in centimeter bands can probe the continuum emission from growing dust grains, ionized winds, and magnetospheric activity, which are in…

astro-ph.SR2016★ 16 cited

The evolutionary status of dense cores in the NGC 1333 IRAS 4 region

E. Koumpia, F. F. S. van der Tak, W. Kwon +3

Protostellar evolution, following the formation of the protostar is becoming reasonably well characterized, but the evolution from a prestellar core to a protostar is not well know…

astro-ph.SR2013★ 244 cited

TADPOL: A 1.3 mm Survey of Dust Polarization in Star-forming Cores and Regions

Charles L. H. Hull, Richard L. Plambeck, Woojin Kwon +22

We present λ1.3 mm CARMA observations of dust polarization toward 30 star-forming cores and 8 star-forming regions from the TADPOL survey. We show maps of all sources, and compare…