| Issue |
A&A
Volume 392, Number 1, September II 2002
|
|
|---|---|---|
| Page(s) | 335 - 339 | |
| Section | Celestial mechanics and astrometry | |
| DOI | https://doi.org/10.1051/0004-6361:20021186 | |
| Published online | 22 August 2002 | |
Visible and near-infrared spectroscopy of the Centaur 32532 (2001 PT
)*
ESO Large Program on TNOs and Centaurs: First spectroscopy results
1
LESIA, Observatoire de Paris, 92195 Meudon Pricipal Cedex, France e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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2
European Southern Observatory ESO, Alonso de Cordova 3107, Santiago de Chile, Chile e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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3
INAF, Osservatorio Astronomico di Torino, Strada Osservatorio 20, 10025 Pino Torinese, Italy e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
4
INAF, Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio Catone, Italy
5
Astronomical Department of Padova, Vicolo dell' Osservatorio 2, 35122 Padova, Italy e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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6
INAF, Osservatorio astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
7
Institute for Astronomy, Universidad Catolica del Norte, Antofagasta, Chile e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
8
Max-Planck-Institut für Astronomie, Königstuhl 17, 69117 Heidelberg, Germany e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
9
IFA, University of Hawaii, 2680 Woodlawn Drive, Honolulu, Hawaii 96822, USA e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
10
Instituto de Astrofisica de Andalucia CSIC, PO Box 3004, 18080 Granada, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
11
National Astronomical Observatory, Osawa 2-21-1, Mitaka, Tokyo, Japan e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
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12
Max-Planck-Institut für Aeronomie, Postfach 20, 37189 Katlenburg-Lindau, Germany e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
13
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching, Germany e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
14
Astronomy Technology Centre, Blackford Hill, Edinburgh EH9 3HJ, UK e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Corresponding author: M. A. Barucci, This email address is being protected from spambots. You need JavaScript enabled to view it.
Received:
6
May
2002
Accepted:
20
June
2002
Abstract
We present photometric and spectroscopic data obtained through visible and near-infrared observations of the Centaur 32532 (2001 PT13) performed with FORS1 and ISAAC at the Very Large Telescope (VLT-ESO) within the framework of an ESO large program on the Trans-Neptunian objects (TNOs) and Centaurs. The results show evidence for a difference in the near-infrared spectral behaviour obtained during two observations carried out one month apart. In one spectrum there is the possible presence of signatures of water ice in small amounts. Two models have been proposed to interpret the surface composition of this Centaur.
Key words: Centaur / 32532 (2001 PT13) / visible / near-infrared / spectroscopy / photometry
Based on observations obtained at the VLT Observatory Cerro Paranal of European Southern Observatory, ESO in Chile within the framework of program 167.C-0340.
© ESO, 2002
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