International audienceObservations show that 100 km class Kuiper Belt objects (KBOs) can be divided into (at least) two color groups, red (R; g - i 1.2), reflecting a difference in their surface composition. This is thought to imply that KBOs formed over a relatively wide range of radial distance, r. The cold classicals at 42 au r*, with 30 au < r* < 40 au. The proposed transition at 30 au < r* < 40 au would explain why the VR objects in the dynamically hot population have smaller orbital inclinations than the R objects, because the orbital excitation from Neptune weakens for orbits starting beyond 30 au. Possible causes of the R-VR color bimodality are discussed
We conducted a two-night photometric survey of small Kuiper Belt objects (KBOs) near opposition usin...
International audienceWe report measurements of the low inclination component of the main Kuiper Bel...
International audienceThe Outer Solar System Origins Survey (OSSOS) has now completed its detailed s...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
International audienceEver since the very first photometric studies of Centaurs and Kuiper belt obje...
Abstract. Ever since the very first photometric studies of Centaurs and Kuiper Belt Objects (KBOs) t...
Dynamically excited objects within the Kuiper Belt show a bimodal distribution in their surface colo...
International audienceThe Colours of the Outer Solar System Origins Survey (Col-OSSOS, Schwamb et al...
Both physical and dynamical properties must be considered to constrain the origins of the dynamicall...
We present new optical broadband colors, obtained with the Keck 1 and Vatican Advanced Technology te...
Ever since the very first photometric studies of Centaurs and Kuiper belt objects (KBOs) t...
Color measurements and albedo distributions introduce non-intuitive observational biases in size-col...
We conducted a two-night photometric survey of small Kuiper Belt objects (KBOs) near opposition usin...
International audienceWe report measurements of the low inclination component of the main Kuiper Bel...
International audienceThe Outer Solar System Origins Survey (OSSOS) has now completed its detailed s...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
A large population of small, icy bodies orbits the sun just beyond Neptune, known as the Kuiper Belt...
As a result of our continuing photometric survey, we report here optical colors for 36 Kuiper Belt o...
International audienceEver since the very first photometric studies of Centaurs and Kuiper belt obje...
Abstract. Ever since the very first photometric studies of Centaurs and Kuiper Belt Objects (KBOs) t...
Dynamically excited objects within the Kuiper Belt show a bimodal distribution in their surface colo...
International audienceThe Colours of the Outer Solar System Origins Survey (Col-OSSOS, Schwamb et al...
Both physical and dynamical properties must be considered to constrain the origins of the dynamicall...
We present new optical broadband colors, obtained with the Keck 1 and Vatican Advanced Technology te...
Ever since the very first photometric studies of Centaurs and Kuiper belt objects (KBOs) t...
Color measurements and albedo distributions introduce non-intuitive observational biases in size-col...
We conducted a two-night photometric survey of small Kuiper Belt objects (KBOs) near opposition usin...
International audienceWe report measurements of the low inclination component of the main Kuiper Bel...
International audienceThe Outer Solar System Origins Survey (OSSOS) has now completed its detailed s...