EB
Edwin Bergin
University of Michigan, University of Massachusetts Amherst, Villanova University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Astrophysics and Star Formation Studies · Stellar, planetary, and galactic studies · Astro and Planetary Science
Employment
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University of Michigan Professor2003 - Present
Education
- 1989 - 1995
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Villanova University B.S.1985 - 1989
Projects & Funding
Projects & funding information is unavailable.
Publications (480)
- The ALMA View of the Edge-on Gomez’s Hamburger System: A Highly Dynamic, Asymmetric Protoplanetary Disk Reveals the Earliest Phases of Giant Planet Formation Save
- Mapping Molecular Ion Distributions in a Diverse Sample of Protoplanetary Disks Save
- Around the water snowline: I. Effects of dynamical and chemical interplay on mid-infrared water spectra of protoplanetary discs Save
- Angular momentum of planet-forming disks: Implications for infall-driven misalignments Save
- Detection of the Polycyclic Aromatic Hydrocarbon Phenalene (C13H10) in the Very Low-luminosity Object MC27/L1521F Save
- JWST/MIRI Hydrocarbon and Water Absorption in the Wind of a Young Disk: Signatures of Pebble Drift and Carbon Grain Sublimation Save
- Water D/H in 3I/ATLAS as a probe of formation conditions in another planetary system Save
- Physical and Chemical Characterization of GY 91’s Multi-ringed Protostellar Disk with ALMA Save
- Investigations of Ultraviolet Spectral Approximations for Computing Photodissociation and Photoionization Reaction Rates Save
- H 2 18 O in the Terrestrial Planet-forming Regions of Protoplanetary Disks Save
- Modeling the Effect of C/O Ratio on Complex Carbon Chemistry in Cold Molecular Clouds Save
- Oxygen Isotope Constraints on the Importance of Photochemical Processing in Protoplanetary Disks Save
- Unveiling the Chemical Complexity and C/O Ratio of the HD 163296 Protoplanetary Disk: Constraints from Multiline ALMA Observations of Organics, Nitriles, and Sulfur-bearing and Deuterated Molecules Save
- Characterizing the physical and chemical properties of the Class I protostellar system Oph-IRS 44 Save
- Soot Planets Instead of Water Worlds Save
- Dust Recycling and Icy Volatile Enhancement (DRIVE): A Novel Method of Volatile Enrichment in Cold Giant Planets Save
- Is cosmic dust porous? Save
- The Molecular Inventory of TMC-1 with GOTHAM Observations Save
- JWST-MIRI Observations of the Irradiated Chemistry in the Inner Disk Cavity of GM Aur Save
- Cosmic Cascades: How Disk Substructure Regulates the Flow of Water to Inner Planetary Systems Save