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2MASS All Sky Catalog of point sources.
A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas
Systematic biases in radiometric diameter determinations
Differentiation of the asteroid Ceres as revealed by its shape
C Ceres has a shape and smoothness indicative of a gravitationally relaxed object that is significantly less flattened than that expected for a homogeneous object, but is consistent with a central mass concentration indicative of differentiation.
VizieR Online Data Catalog: 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)
Photometric analysis of 1 Ceres and surface mapping from HST observations
Cometary dust trails: I. Survey
The Formation of Encke Meteoroids and Dust Trail
Abstract We observed Comet 2P/Encke with the Infrared Space Observatory ISOCAM on July 14, 1997, from a particularly favorable viewing geometry above the comet's orbital plane and at a distance of…
Origin of the Near-Ecliptic Circumsolar Dust Band
- D. Nesvorný, W. Bottke, D. Vokrouhlický, M. Sykes, D. Lien, J. Stansberry
- Physics, Geology
- 1 June 2008
The zodiacal dust bands are bright infrared (IR) strips produced by thermal emission from circumsolar rings of particles. Two of the three principal dust bands, known as β and γ, were previously…