“TNOs are Cool”: A survey of the trans-Neptunian region - X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations

@article{Vilenius2014TNOsAC,
  title={“TNOs are Cool”: A survey of the trans-Neptunian region - X. Analysis of classical Kuiper belt objects from Herschel and Spitzer observations},
  author={E. Vilenius and C. Kiss and T. Muller and Michael Mommert and P. Santos-Sanz and A. P'al and J. Stansberry and M. Mueller and N. Peixinho and E. Lellouch and S. Fornasier and A. Delsanti and A. Thirouin and J. Ortiz and R. Duffard and D. Perna and F. I. F. Physik and H Germany and K. Observatory and R. C. F. Astronomy and Earth Sciences and Hungary. and Deutsches Zentrum fur Luft- und Raumfahrt e.V. and Institute of planetary Research and Northern Arizona University and D. Physics and Astronomy and Usa and Inst. de Astrof'isica de Andaluc'ia and Spain. and L. Paris and Cnrs and Upmc Univ. and France. and S. Observatory and The University of Arizona and Sron Netherlands Institute for Space Research and Netherlands and UNS-CNRS-Observatoire de la Cote d'Azur and Geophysical and Astronomical Observatory of the University of Coimbra and Portugal and U. D. Astronom'ia and Facultad de Ciencias B'asicas and Universidad de Antofagasta and Chile. and U. Diderot and Laboratoire d'Astrophysique de Marseille and U. Provence},
  journal={Astronomy and Astrophysics},
  year={2014},
  volume={564},
  pages={1-18}
}
Context. The Kuiper belt is formed of planetesimals which failed to grow to planets and its dynamical structure has been affected by Neptune. The classical Kuiper belt contains objects both from a low-inclination, presumably primordial, distribution and from a high-inclination dynamically excited population. Aims. Based on a sample of classical trans-Neptunian objects (TNOs) with observations at thermal wavelengths we determine radiometric sizes, geometric albedos and thermal beaming factors… Expand
The color and binarity of (486958) 2014 MU69 and other long-range New Horizons Kuiper Belt targets
Trans-Neptunian objects and Centaurs at thermal wavelengths
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