Richard Teague

Assistant Professor

Massachusetts Institute of Technology

United States

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About

Richard Teague is an Assistant Professor at the Massachusetts Institute of Technology in the United States. His research primarily focuses on protoplanetary disks, kinematic structures, and the mapping of astronomical phenomena, as reflected in his recent articles. His work includes studies on high-redshift quasars, magnetic fields in accretion disks, and variations in elemental fractionation within planet-hosting disks.

Articles (28)

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Collaborators (22)

Jaehan Bae

Assistant Professor

University of Florida

UNITED STATES

Richard Teague

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Articles (28)

The Light Echo of a High-redshift Quasar Mapped with Lyα Tomography

exoALMA. XVIII. Interpreting Large-scale Kinematic Structures as Moderate Warping

A Radially Resolved Magnetic Field Threading the Disk of TW Hya

Radial variations in the nitrogen, carbon, and hydrogen fractionation in the PDS 70 planet-hosting disk

exoALMA. I. Science Goals, Project Design, and Data Products

exoALMA. II. Data Calibration and Imaging Pipeline

exoALMA. III. Line-intensity Modeling and System Property Extraction from Protoplanetary Disks

exoALMA. V. Gaseous Emission Surfaces and Temperature Structures

exoALMA. X. Channel Maps Reveal Complex 12CO Abundance Distributions and a Variety of Kinematic Structures with Evidence for Embedded Planets

exoALMA. XIV. Gas Surface Densities in the RX J1604.3−2130 A Disk from Pressure-broadened CO Line Wings

The Carbon Isotopic Ratio and Planet Formation

On Kinematic Measurements of Self-gravity in Protoplanetary Disks

Constraining the stellar masses and origin of the protostellar VLA 1623 system

ALMA high-resolution observations unveil planet formation shaping molecular emission in the PDS 70 disk

Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk

High turbulence in the IM Lup protoplanetary disk

Outflow Driven by a Protoplanet Embedded in the TW Hya Disk

The First Spatially Resolved Detection of 13CN in a Protoplanetary Disk and Evidence for Complex Carbon Isotope Fractionation

Cold Deuterium Fractionation in the Nearest Planet-forming Disk

Molecules with ALMA at Planet-forming Scales (MAPS): Complex Kinematics in the AS 209 Disk Induced by a Forming Planet and Disk Winds

Mapping Protoplanetary Disk Vertical Structure with CO Isotopologue Line Emission

Constraining the gas distribution in the PDS 70 disc as a method to assess the effect of planet-disc interactions

Tentative co-orbital submillimeter emission within the Lagrangian region L5 of the protoplanet PDS 70 b

A kinematically detected planet candidate in a transition disk

Implications for Chondrule Formation Regions and Solar Nebula Magnetism from Statistical Reanalysis of Chondrule Paleomagnetism

Erratum: “The TW Hya Rosetta Stone Project. I. Radial and Vertical Distributions of DCN and DCO+” (2021, AJ, 161, 38)

A kinematic excess in the annular gap and gas-depleted cavity in the disc around HD 169142

A Localized Kinematic Structure Detected in Atomic Carbon Emission Spatially Coincident with a Proposed Protoplanet in the HD 163296 Disk

Collaborators (22)

Jaehan Bae

Stefano Facchini

Yuhito Shibaike

Takashi Tsukagoshi

L. Ilsedore Cleeves

Gianni Cataldi

GIUSEPPE LODATO

Ian Czekala

Iain Hammond

Bayron Portilla-Revelo

Joseph Hennawi

Seokho Lee

Gabriel Brammer

Inga Kamp

Daniel Price

Sean Andrews

Christian Rab

Teresa Paneque-Carreno

Charles Law

Paola Pinilla

Edwin Bergin

Kenji Furuya

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