"TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)

@article{Mueller2010TNOsAC,
  title={"TNOs are Cool": A survey of the trans-Neptunian region I. Results from the Herschel science demonstration phase (SDP)},
  author={Thomas G. Mueller and Emmanuel Lellouch and J. Stansberry and Cs. P. Kiss and Pablo Santos-Sanz and Esa Vilenius and Silvia Protopapa and Roxana Moreno and M. Mueller and Audrey C. Delsanti and Ren{\'e} Duffard and Sonia Fornasier and O.Groussin and Alan W. Harris and Florence Henry and Jonathan Horner and Pedro Lacerda and Tanya L. Lim and Michael Mommert and Jos{\'e} Luis Ortiz and Miriam Rengel and Audrey Thirouin and D. E. Trilling and Antonella Barucci and Jacques Crovisier and Alain Doressoundiram and Elisabetta Dotto and Pedro J. Guti{\'e}rrez and Olivier R. Hainaut and Paul Hartogh and D. Hestroffer and Mark Richard Kidger and L. M. Lara and Bruce M. Swinyard and Nicolas Thomas},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={518},
  pages={1-5}
}
The goal of the Herschel Open Time Key programme "TNOs are Cool!" is to derive the physical and thermal properties for a large sample of Centaurs and trans-Neptunian objects (TNOs), including resonant, classical, detached and scattered disk objects. We present results for seven targets either observed in PACS point-source, or in mini scan-map mode. Spitzer-MIPS observations were included for three objects. The sizes of these targets range from 100 km to almost 1000 km, five have low geometric… 

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References

SHOWING 1-10 OF 30 REFERENCES

``TNOs are Cool'': A survey of the trans-Neptunian region . III. Thermophysical properties of 90482 Orcus and 136472 Makemake

Context. The goal of the Herschel open time programme “TNOs are Cooll” is to derive the physical and thermal properties for a large sample of Centaurs, and trans-Neptunian objects (TNOs), including

ESO Large Program on physical studies of Trans-Neptunian objects and Centaurs: Final results of the visible spectrophotometric observations

The Large Program on physical studies of TNOs and Centaurs, started at ESO Cerro Paranal on April 2001, has recently been concluded. This project was devoted to the investigation of the surface

Visible and near-infrared colors of Transneptunian objects and Centaurs from the second ESO large program

Aims. We investigate color properties and define or check taxonomic classifications of objects observed in our survey. Methods. All observations were performed between October 2006 and September 2007

Time-resolved Photometry of Kuiper Belt Objects: Rotations, Shapes, and Phase Functions

We present a systematic investigation of the rotational light curves of trans-Neptunian objects based on extensive optical data from Mauna Kea. Four of 13 objects (corresponding to 31%) in our sample

Colors and taxonomy of Centaurs and trans-Neptunian objects

Context. The study of the surface properties of Centaurs and trans-Neptunian objects (TNOs) provides essential information about the early conditions and evolution of the outer Solar System. Due to