Triaxial ellipsoid dimensions and poles of asteroids from AO observations at the Keck-II telescope
暂无分享,去创建一个
[1] Thierry Fusco,et al. Physical Properties of (2) Pallas , 2009, 0912.3626.
[2] J. Christou,et al. Triaxial ellipsoid dimensions and rotational poles of seven asteroids from Lick Observatory adaptive optics images, and of Ceres , 2008 .
[3] Thierry Fusco,et al. Near-Infrared Mapping and Physical Properties of the Dwarf-Planet Ceres , 2007, 0711.1152.
[4] M. Birlan,et al. New determination of the size and bulk density of the binary Asteroid 22 Kalliope from observations of mutual eclipses , 2007, 0710.1471.
[5] C. Chapman,et al. Discovery of an Extreme Mass-Ratio Satellite of (41) Daphne in a Close Orbit , 2008 .
[6] A. Harris,et al. New findings on asteroid spin-vector distributions , 2007 .
[7] Thierry Fusco,et al. Direct measurement of the size, shape, and pole of 511 Davida with Keck AO in a single night , 2007 .
[8] J Berthier,et al. Shape, size and multiplicity of main-belt asteroids I. Keck Adaptive Optics survey. , 2006, Icarus.
[9] Jack D. Drummond,et al. Measurements of Binary Stars, Including Two New Discoveries, with the Lick Observatory Adaptive Optics System , 2006 .
[10] Daniel Hestroffer,et al. Mass and density of Asteroid 121 Hermione from an analysis of its companion orbit , 2005 .
[11] Mikko Kaasalainen,et al. Shapes and rotational properties of thirty asteroids from photometric data , 2003 .
[12] M. Kaasalainen,et al. Models of Twenty Asteroids from Photometric Data , 2002 .
[13] Karri Muinonen,et al. Optimization Methods for Asteroid Lightcurve Inversion. II. The Complete Inverse Problem , 2001 .
[14] M. Kaasalainen,et al. Optimization Methods for Asteroid Lightcurve Inversion: I. Shape Determination , 2001 .
[15] J. Drummond. Measuring Asteroids with Adaptive Optics , 2000 .
[16] N. Ageorges,et al. Laser guide star adaptive optics for astronomy , 2000 .
[17] M. Kaasalainen,et al. Optimization methods for asteroid lightcurve inversion , 1999 .
[18] C. Blanco,et al. POLE COORDINATES AND SHAPE OF 30 ASTEROIDS , 1998 .
[19] Jack D. Drummond. Adaptive optics Lorentzian point spread function , 1998, Astronomical Telescopes and Instrumentation.
[20] P. Denchev,et al. Models of Four Asteroids: 17 Thetis, 52 Europa, 532 Herculina, and 704 Interamnia , 1995 .
[21] T. Michałowski. Poles, Shapes, Senses of Rotation, and Sidereal Periods of Asteroids , 1993 .
[22] T. Kwiatkowski,et al. Spin vector and shape of 532 Herculina , 1992 .
[23] R. Binzel,et al. The size and shape of (2) Pallas from the 1983 occultation of 1 Vulpeculae , 1990 .
[24] J. Surdej,et al. Asteroid 532 Herculina - Lightcurves, pole orientation and a model , 1987 .
[25] E. Hege,et al. Speckle interferometry of asteroids: I. 433 eros , 1985 .
[26] N. White,et al. The diameter of Pallas from its occultation of SAO 85009 , 1979 .