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809 Lundia
On the V-Type Asteroids Outside the Vesta Family. I. Interplay Of
Dynamical Erosion of the Asteroid Belt and Implications for Large Impacts in the Inner Solar System
List of Scientific Presentations
Asteroid Regolith Weathering: a Large-Scale Observational Investigation
The Minor Planet Bulletin
Multiple Asteroid Systems: Dimensions and Thermal Properties from Spitzer Space Telescope and Ground-Based Observations Q ⇑ F
Characterization of Asteroids and Tnos Authors: T
Asteroid Family Physical Properties, Numerical Sim- Constraints on the Ages of Families
1 Collisions History in the Main-Belt by Spectroscopic
A New Non-Convex Model of the Binary Asteroid (809) Lundia Obtained with the SAGE Modelling Technique
On the V-Type Asteroids Outside the Vesta Family
New Binary Asteroid 809 Lundia I
The Minor Planet Bulletin
Summary of Professional Accomplishments
Techniques for Asteroid Spectrocopy Marcel Popescu
Academia Român˘A Institutul Astronomic Bucure ¸Sti
Demeo.Icarus.2019.Pdf
Non-Vestoid Candidate Asteroids in the Inner Main Belt Therefore Ruling out Its Vestoidal Origin
Top View
Oxygen and Asteroids Thomas H
Catalogue of Minor Planet Names and Discovery Circumstances
Do Slivan States Exist in the Flora Family? I
PDF Hosted at the Radboud Repository of the Radboud University Nijmegen
Physical Characterization of Equal-Mass Binary Near-Earth Asteroid 2017 YE5: a Possible Dormant Jupiter-Family Comet
LIGHTCURVE of 755 QUINTILLA the Nightly Zero-Point Was Determined by Imaging a Landolt Standard Field That Was Fortuitously Only a Few Degrees Away from Robert K
Abstracts 181-184 (2008)
Identification and Dynamical Properties of Asteroid Families
Differentiation Signatures in the Flora Region
Non-Convex Model of the Binary Asteroid (809) Lundia and Its Density Estimation
Minor Planet Names: Alphabetical List