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755 Quintilla
Binzel, RP (2002). “Phase II of the Small Main-Belt Asteroid
Spectroscopic Survey of X-Type Asteroids S
1 PRELIMINARY SPIN-SHAPE MODEL for 755 QUINTILLA Lorenzo Franco Balzaretto Observatory (A81), Rome, ITALY Lor
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Cumulative Index to Volumes 1-45
Near-Infrared Spectroscopic Analysis of Mainbelt M-Asteroid 755 Quintilla
Spectroscopic Survey of M-Type Asteroids S
Appendix a Appendix A
The Thousand Asteroid Light Curve Survey
242 Minor Planet Bulletin 47 (2020) COLLABORATIVE ASTEROID
University Microfilms International 300 N
LIGHT CURVE of 755 QUINTILLA Robert K
Departmental Plan for Assessment of Student Learning ***Revised
JRASC August 2006, High Resolution (PDF)
Timothy R. Young 1. Education 2. Professional Experience
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
Spectroscopic Survey of M--Type Asteroids
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