EDP Sciences
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This article is an erratum for: [this article]

Volume 495, Number 3, March I 2009
Page(s) 899 - 900
Section Interstellar and circumstellar matter
DOI http://dx.doi.org/10.1051/0004-6361/20077899e
Published online 09 February 2009
A&A 495, 899-900 (2009)
DOI: 10.1051/0004-6361/20077899e


Results from DROXO

I. The variability of fluorescent Fe 6.4 keV emission in the young star Elias 29. High-energy electrons in the star's accretion tubes?
G. Giardino1, F. Favata2, I. Pillitteri3, E. Flaccomio3, G. Micela3, and S. Sciortino3

1  ESA – Research and Science Support Department, ESTEC, Postbus 299, 2200 AG Noordwijk, The Netherlands
    e-mail: ggiardin@rssd.esa.int
2  ESA – Planning and Community Coordination Office, Science Programme, 8–10 rue Mario Nikis, 75738 Paris Cedex 15, France
3  INAF – Osservatorio Astronomico di Palermo, Piazza del Parlamento 1, 90134 Palermo, Italy

Without abstract

Key words: ISM: clouds -- ISM: individual objects: $\rho$-Oph cloud -- stars: pre-main sequence -- X-rays: stars -- stars: individual: Elias 29 -- Errata, addenda

© ESO 2009
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