Volume 373, Number 3, July III 2001
|Page(s)||L29 - L32|
|Published online||15 July 2001|
NICS-TNG infrared spectroscopy of trans-neptunian objects 2000 EB173 and 2000 WR106
Centro Galileo Galilei & Telescopio Nazionale Galileo, PO Box 565, 38700, S/C de La Palma, Tenerife, Spain
2 Osservatorio di Arcetri, Largo E. Fermi 5, 50125 Firenze, Italy
3 Osservatorio Astronomico di Torino, 10025 Pino Torinese, Italy
Corresponding author: J. Licandro, email@example.com
Accepted: 25 May 2001
We report complete near-infrared (0.9-2.4 μm) spectral observations of trans-neptunian objects (TNOs) 2000 EB173 and 2000 WR106 collected using the new Near Infrared Camera Spectrometer (NICS) attached to the 3.56 m Telescopio Nazionale Galileo (TNG). Both spectra are very red and with a quite strong and broad drop extending throughout the K band. However, while 2000 EB173 does not show any evidence of narrow absorption features, the spectrum of 2000 WR106 has quite deep water ice absorption at 1.5 and 2.0 μm. Moreover, the latter object is significantly less red than the former indicating, therefore, that the surface of 2000 WR106 is "cleaner" (i.e. less processed by particle irradiation) than that of 2000 EB173.
Key words: minor planets / comets / infrared / trans-neptunian objects
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.