Bruce Draine

Professor

Princeton University

United States

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About

Bruce Draine is a Professor at Princeton University in the United States. His research focuses on astrophysical subjects, including the behavior of polycyclic aromatic hydrocarbons, interstellar dust properties, and the impacts of active galactic nuclei on galaxy emissions. Recent publications include investigations into the metallicity dependence of PAH emission and the detection of deuterated hydrocarbon nanoparticles in the Whirlpool Galaxy.

Articles (18)

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2025

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2021

Collaborators (9)

Brandon S Hensley

Princeton University

UNITED STATES

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Konstantin Herbst

Lecturer

Christian-Albrechts-Universität zu Kiel

GERMANY

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John-David Smith

University of Toledo

UNITED STATES

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Christopher Packham

University of Texas at San Antonio

UNITED STATES

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Jamey R. Szalay

UNITED STATES

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Mihály Horányi

UNITED STATES

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Charles M. Telesco

Professor

University of Florida

UNITED STATES

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Francoise Combes

Professor

FRANCE

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Cory Whitcomb

University of California, San Diego

UNITED STATES

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Bruce Draine

Research Interests

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About

Articles (18)

Erratum: “Excitation of Polycyclic Aromatic Hydrocarbon Emission: Dependence on Size Distribution, Ionization, and Starlight Spectrum and Intensity” (2021, ApJ, 917, 3)

The Spheroidal Analog Method for Modeling Irregular Porous Aggregates

Detection of Deuterated Hydrocarbon Nanoparticles in the Whirlpool Galaxy, M51

The Impact of an Active Galactic Nucleus on Polycyclic Aromatic Hydrocarbon Emission in Galaxies: The Case of Ring Galaxy NGC 4138

The Metallicity Dependence of PAH Emission in Galaxies. I. Insights from Deep Radial Spitzer Spectroscopy

Sensitivity of Polarization to Grain Shape. II. Aggregates

Erratum: “Observational Constraints on the Physical Properties of Interstellar Dust in the Post-Planck Era” (2021, ApJ, 906, 73)

Sensitivity of Polarization to Grain Shape. I. Convex Shapes

Gas, dust, and the CO-to-molecular gas conversion factor in low-metallicity starbursts

Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers)

The Astrodust+PAH Model: A Unified Description of the Extinction, Emission, and Polarization from Dust in the Diffuse Interstellar Medium

Erratum: “Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains” (2021, ApJ, 919, 65)

Mid-infrared Polarization of the Diffuse Interstellar Medium toward CygOB2-12

Dust in and Around the Heliosphere and Astrospheres

An Optical Spectrum of the Diffuse Galactic Light from BOSS and IRIS

On Far-infrared and Submillimeter Circular Polarization

Excitation of Polycyclic Aromatic Hydrocarbon Emission: Dependence on Size Distribution, Ionization, and Starlight Spectrum and Intensity

Using the Starlight Polarization Efficiency Integral to Constrain Shapes and Porosities of Interstellar Grains

Collaborators (9)

Brandon S Hensley

Konstantin Herbst

John-David Smith

Christopher Packham

Jamey R. Szalay

Mihály Horányi

Charles M. Telesco

Francoise Combes

Cory Whitcomb

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