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434 Hungaria
Dynamical Evolution of the Hungaria Asteroids ⇑ Firth M
The Hungaria Asteroids: Close Encounters and Impacts with Terrestrial Planets
Hungaria Asteroid Family As the Source of Aubrite Meteorites
Mineralogical Variations Among High Albedo E-Type Asteroids: Implications for Asteroid Igneous Processes
2-Meter Diameter Near-Earth Asteroid 2015 TC25: a Possible Boulder from E-Type Asteroid (44) Nysa
Visible and Near Infrared Spectroscopic Investigation of E-Type Asteroids, Including 2867 Steins, a Target of the Rosetta Mission S
Radar Observations of E-Class Asteroids 44 Nysa and 434 Hungaria
The Full Appendices with All References
Are the E-Type Asteroids (2867) Steins, a Target of the Rosetta Mission, and NEA (3103) Eger Remnants of an Old Asteroid Family?
Polarimetric Observations of Hungaria Asteroids
Demeo.Icarus.2019.Pdf
Supplementary Information
Dynamics of the Hungaria Asteroids
An Unusual E-Type Asteroid
Mineralogy and Surface Composition of Asteroids Vishnu Reddy Planetary Science Institute
Near-Earth Asteroid Surface Roughness Depends on Compositional Class ∗ Lance A.M
One of Everything: the Breakthrough Listen Exotica Catalog
Oxygen and Asteroids Thomas H
Top View
Mineralogy and Surface Composition of Asteroids
The Minor Planet Bulletin
Minor Planet Names: Alphabetical List