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250 Bettina
An Ancient and a Primordial Collisional Family As the Main Sources of X-Type Asteroids of the Inner Main Belt
Asteroid Observations at Low Phase Angles. IV. Average Parameters for the New H, G1, G2 Magnitude System Vasilij G
The Minor Planet Bulletin Is Continuing in Were Conducted on 2004 UT Dates March 26 and 30 and April 7 Printed Form
Spectroscopic Survey of M-Type Asteroids S
The International Conference on Asteroids, Comets, Meteors 1991
BAA Handbook
Spectroscopy of K-Complex Asteroids: Parent Bodies of Carbonaceous Meteorites? ∗ Beth Ellen Clark A, ,1, Maureen E
University Microfilms International 300 N
Study of Ephemeris Accuracy of the Minor Planets
Composition and Origin of L5 Trojan Asteroids of Mars
The Composition of M-Type Asteroids II: Synthesis of Spectroscopic and Radar Observations
Plausible Parent Bodies for Enstatite Chondrites and Mesosiderites: Implications for Lutetia’S Fly-By P
The International Conference on Asteroids, Comets, Meteors 1991
The Minor Planet Bulletin (Warner Et Al., 2008)
Ancient and Primordial Collisional Families As the Main Sources of X-Type Asteroids of the Inner Main Belt
The Minor Planet Bulletin, 30(3), Pp
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