Light curves of 5 Trans-Neptunian Objects

DOI

Trans-Neptunian objects (TNOs) represent a new frontier in the study of our Solar System. In particular, the investigation of their rotational properties can provide important hints about their internal structure and collisional evolution. We expand the limited sample of TNOs with known rotation rates, and improve the knowledge of the physical nature of these bodies.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35080451
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/508/451
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/508/451
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/508/451
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/508/451
Provenance
Creator Perna D.; Dotto E.; Barucci; M.A.; Rossi A.; Fornasier S.; de Bergh C.
Publisher CDS
Publication Year 2010
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Solar System Astronomy