A&A 487, 1195-1196 (2008)
DOI: 10.1051/0004-6361:20078340e

Erratum

Spectral properties of asteroids in cometary orbits

J. Licandro1 - A. Alvarez-Candal2,[*] - J. de León1 - N. Pinilla-Alonso3 - D. Lazzaro2 - H. Campins4,5


1 - Instituto de Astrofísica de Canarias, c/Vía Láctea s/n, 38205, La Laguna, Tenerife, Spain
2 - Observatório Nacional - MCT. Rua Gal. José Cristino 77, Rio de Janeiro, 20921-400 RJ, Brazil
3 - Fundación Galileo Galilei & Telescopio Nazionale Galileo, PO Box 565, 38700, S/C de La Palma, Tenerife, Spain
4 - Physics Department, University of Central Florida, Orlando, FL, 32816, USA
5 - LPL, University of Arizona, Tucson Az, 85721, USA

A&A 481, 861-877 (2008), DOI: 10.1051/0004-6361:20078340


Key words: minor planets, asteroids - comets: general - methods: observational - techniques: spectroscopic - errata, addenda


The spectra printed in the second column of Fig. 1 are the same as in the first column. The corrected figure is reproduced here. The error does not affect the argumentation and conlusions of the paper.


  \begin{figure}\includegraphics[height=8.5cm,width=19cm,angle=-90,clip]{8340fig1}...
...
\includegraphics[height=8.5cm,width=19cm,angle=-90,clip]{8340fig2}\end{figure} Figure 1: Near-infrared reflectance spectra of the asteroids, normalized at 1.0 $\mu $m. Spectra are shifted in reflectance for clarity.
Open with DEXTER



Copyright ESO 2008