Q. Daniel Wang

Professor

University of Massachusetts Amherst

United States

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About

Q. Daniel Wang is a Professor at the University of Massachusetts Amherst in the United States. His research focuses on astrophysics, particularly in the areas of galaxy clusters, X-ray emissions, and accretion flows in black holes. He has published extensively on topics such as the discovery of young clusters of galaxies, the characteristics of diffuse X-ray emissions, and the dynamics of molecular gas in galactic winds.

Articles (25)

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2022

Collaborators (10)

Joel Bregman

H.D. Curtis Professor of Astronomy

University of Michigan

UNITED STATES

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Hsiao-Wen Chen

Professor

University of Chicago

UNITED STATES

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Mark Heyer

Research Professor

University of Massachusetts Boston

UNITED STATES

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N M McClure-Griffiths

Australian National University

AUSTRALIA

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Lister Staveley-Smith

University of Western Australia

AUSTRALIA

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Min Long

Assistant Professor

Boise State University

UNITED STATES

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Filippo Fraternali

University of Groningen

NETHERLANDS

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Judith Irwin

Professor

Queen's University

CANADA

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Luca Cortese

University of Western Australia

AUSTRALIA

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Min Yun

University of Massachusetts Amherst

UNITED STATES

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Q. Daniel Wang

Research Interests

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Articles (25)

Cold molecular gas in the hot nuclear wind of the Milky Way

Serendipitous Discovery of a Young Cluster of Galaxies at z ∼ 0.5 Projected Next to the Nearby Tadpole Galaxy KUG 1138 + 327

Diffuse X-Ray Emission in M51: A Hierarchical Bayesian Spatially Resolved Spectral Analysis

Candidate Intermediate-mass Black Hole Discovered in an Extremely Young Low-metallicity Cluster in the Tadpole Galaxy KUG 1138+327

CO-CHANGES

CHANG-ES. XXXV. Cosmic Ray Transport and Magnetic Field Structure of NGC 3556 at 3 GHz

CHANG-ES. XXXII. Spatially Resolved Thermal–Nonthermal Separation from Radio Data Alone—New Probes into NGC 3044 and NGC 5775

FEASTS Combined with Interferometry. I. Overall Properties of Diffuse H i and Implications for Gas Accretion in Nearby Galaxies

CHANG-ES. XXX. 10 kpc Radio Lobes in the Sombrero Galaxy

PASSAGES: The Wide-ranging, Extreme Intrinsic Properties of Planck-selected, Lensed Dusty Star-forming Galaxies

CHANG-ES

Multistructured Accretion Flow of Sgr A*. I. Examination of a Radiatively Inefficient Accretion Flow Model

Multistructured Accretion Flow of Sgr A*. II. Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds

The X-ray variation of M81* resolved by <i>Chandra</i> and <i>NuSTAR</i>

Tracing the Energetic Outflows from Galactic Nuclei: Observational Evidence for a Large-Scale Bipolar Radio and X-ray-emitting Bubble-like Structure in M106

An XMM-Newton View of the Andromeda Galaxy as Explored in a Legacy Survey (New-ANGELS). I. The X-Ray Source Catalog

CO-CHANGES I: IRAM 30m CO Observations of Molecular Gas in the Sombrero Galaxy

FEASTS: IGM Cooling Triggered by Tidal Interactions through the Diffuse H i Phase around NGC 4631

X-ray detection of the most extreme star-forming galaxies at the cosmic noon via strong lensing

X-Rays Trace the Volatile Content of Interstellar Objects

X-Ray Spectroscopic Evidence of Charge Exchange Emission in the Disk of M51

Correction to: ‘Decomposing magnetic fields in three dimensions over the central molecular zone’

Statistical properties of cataclysmic variables in the local galactic disc: a joint analysis of Gaia and XMM–Newton data

PASSAGES: the Large Millimeter Telescope and ALMA observations of extremely luminous high-redshift galaxies identified by the Planck

CHANG-ES XXIX: the sub-kpc nuclear bubble of NGC 4438

Collaborators (10)

Joel Bregman

Hsiao-Wen Chen

Mark Heyer

N M McClure-Griffiths

Lister Staveley-Smith

Min Long

Filippo Fraternali

Judith Irwin

Luca Cortese

Min Yun

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