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A&A 410, L29-L32 (2003)
DOI: 10.1051/0004-6361:20031420
Letter
Reopening the TNOs color controversy: Centaurs bimodality and TNOs unimodality
N. Peixinho1, 2, A. Doressoundiram1, A. Delsanti1, H. Boehnhardt3, M. A. Barucci1 and I. Belskaya1, 41 LESIA, Observatoire de Paris, 5 Pl. Jules Janssen, 92195 Meudon Cedex, France
e-mail: Nuno.Peixinho@obspm.fr;
e-mail: Nuno.Peixinho,Alain.Doressoundiram,Antonella.Barucci@obspm.fr
2 CAAUL, Observatório Astronómico de Lisboa, Tapada da Ajuda, 1349-018 Lisboa, Portugal
3 Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany
e-mail: hboehnha@mpia-hd.mpg.de
4 Astronomical Observatory of Kharkov National University, Sumskaya St. 35, Kharkov 61022, Ukraine
e-mail: irina@astron.kharkov.ua
(Received 8 August 2003 / Accepted 12 September 2003 )
Abstract
We revisit the Trans-Neptunian Objects (TNOs) color
controversy allegedly solved by Tegler & Romanishin (2003). We debate the
statistical approach of the quoted work and discuss why it can not
draw the claimed conclusions, and reanalyze their data sample with a
more adequate statistical test. We find evidence for the existence of
two color groups among the Centaurs. Therefore, mixing both centaurs
and TNOs populations lead to the erroneous conclusion of a global
bimodality, while there is no evidence for two color groups in the
TNOs population alone. We use quasi-simultaneous visible color
measurements published for 20 centaurs (corresponding to about half of
the identified objects of this class), and conclude on the existence
of two groups. With the surface evolution model of Delsanti et al. (2003). we
discuss how the existence of two groups of Centaurs may be compatible
with a continuous TNOs color distribution.
Key words: Kuiper Belt -- methods: statistical
Offprint request: N. Peixinho, Nuno.Peixinho@obspm.fr
© ESO 2003
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