Ke Zhang

Assistant Professor

University of Wisconsin-Madison

United States

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About

Dr. Ke Zhang is an Assistant Professor at the University of Wisconsin-Madison, USA. His research primarily focuses on protoplanetary disks, exploring the evolution of gas and dust within these systems. Recent publications include a series of articles on the ALMA Survey of Gas Evolution of Protoplanetary Disks (AGE-PRO), where he investigates disk properties across various star-forming regions.

Articles (20)

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2021

Collaborators (9)

Ardjan Sturm

Leiden University

NETHERLANDS

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Colette Salyk

Assistant Professor

Vassar College

UNITED STATES

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Melissa McClure

Assistant Professor

Leiden University

NETHERLANDS

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L. Ilsedore Cleeves

University of Virginia

UNITED STATES

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Zhaohuan Zhu

University of Nevada

UNITED STATES

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Till Kaeufer

University of Exeter

UNITED KINGDOM

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Cristobal Petrovich

Associate Professor

Indiana State University

UNITED STATES

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Paola Pinilla

Associate Professor

UNITED KINGDOM

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Edwin Bergin

Professor

University of Michigan

UNITED STATES

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Ke Zhang

Research Interests

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About

Articles (20)

Cosmic Cascades: How Disk Substructure Regulates the Flow of Water to Inner Planetary Systems

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). I. Program Overview and Summary of First Results

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). II. Dust and Gas Disk Properties in the Ophiuchus Star-forming Region

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). III. Dust and Gas Disk Properties in the Lupus Star-forming Region

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). IV. Dust and Gas Disk Properties in the Upper Scorpius Star-forming Region

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). V. Protoplanetary Gas Disk Masses

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). VI. Comparison of Dust Evolution Models to AGE-PRO Observations

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). VIII. The Impact of External Photoevaporation on Disk Masses and Radii in Upper Scorpius

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). X. Dust Substructures, Disk Geometries, and Dust-disk Radii

The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO). XI. Beam-corrected Gas Disk Sizes from Fitting 12CO Moment Zero Maps

Substructures in Compact Disks of the Taurus Star-forming Region

How Large Is a Disk—What Do Protoplanetary Disk Gas Sizes Really Mean?

A Gap-sharing Planet Pair Shaping the Crescent in HD 163296: A Disk Sculpted by a Resonant Chain

New Constraints on Protoplanetary Disk Gas Masses in Lupus

Hydrostatic Equilibrium Does Not Solve the C18O Flux Problem in Protoplanetary Disks

A Novel Way of Measuring the Gas Disk Mass of Protoplanetary Disks Using N2H+ and C18O

Effect of MHD Wind-driven Disk Evolution on the Observed Sizes of Protoplanetary Disks

Molecules with ALMA at Planet-forming Scales (MAPS). V. CO Gas Distributions

Molecules with ALMA at Planet-forming Scales (MAPS). VII. Substellar O/H and C/H and Superstellar C/O in Planet-feeding Gas

Molecules with ALMA at Planet-forming Scales (MAPS). VIII. CO Gap in AS 209—Gas Depletion or Chemical Processing?

Collaborators (9)

Ardjan Sturm

Colette Salyk

Melissa McClure

L. Ilsedore Cleeves

Zhaohuan Zhu

Till Kaeufer

Cristobal Petrovich

Paola Pinilla

Edwin Bergin

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