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110 Lydia
Perturbations in the Motion of the Quasicomplanar Minor Planets For
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And X-Class Asteroids. II. Summary and Synthesis
IRTF Spectra for 17 Asteroids from the C and X Complexes: a Discussion of Continuum Slopes and Their Relationships to C Chondrites and Phyllosilicates ⇑ Daniel R
(2000) Forging Asteroid-Meteorite Relationships Through Reflectance
Thermal Inertia of Main Belt Asteroids Smaller Than 100 Km from IRAS Data
Cumulative Index to Volumes 1-45
M-Asteroids: Searching for Weak Silicate Features on Potentially Differentiated Objects
New and Updated Convex Shape Models of Asteroids Based on Optical Data from a Large Collaboration Network
Observer's Handbook 1981
Spectroscopic Survey of M-Type Asteroids S
The Composition of M-Type Asteroids: Synthesis of Spectroscopic and Radar Observations
The Minor Planet Bulletin (Warner Et Al., 2009A)
The Minor Planet Bulletin
Exogenous Origin of Hydration on Asteroid (16) Psyche: the Role of Hydrated Asteroid Families
DAMIT: a Database of Asteroid Models
Characterization of Thermal Inertia
University Microfilms International 300 N
Top View
Oxygen and Asteroids Thomas H
Study of Ephemeris Accuracy of the Minor Planets
1971Aj 76. . 14It the Astronomical Journal
The Composition of M-Type Asteroids II: Synthesis of Spectroscopic and Radar Observations
The Complete Guide to Observing Lunar, Grazing and Asteroid Occultations
Thermal Inertia of Main Belt Asteroids Smaller Than 100 Km from IRAS Data Marco Delbo, Paolo Tanga
The Minor Planet Bulletin 40 (2013) 65
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REMOTE SENSING of SMALL BODIES 1:30 P.M
The Frick Collection Members’ Magazine Winter 2008
Astrometric Asteroid Masses: a Simultaneous Determination
Minor Planet Names: Alphabetical List