Line formation in solar granulation

M. Asplund; N. Grevesse; A. J. Sauval; C. Allende Prieto; D. Kiselman

doi:10.1051/0004-6361:20034328e

Free Access

Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 435, Number 1, May III 2005


Page(s)		339 - 340
Section		The Sun
DOI		https://doi.org/10.1051/0004-6361:20034328e
Published online		25 April 2005

A&A 435, 339-340 (2005)

IV. [O I], O I and OH lines and the photospheric O abundance

M. Asplund¹, N. Grevesse²^,3, A. J. Sauval⁴, C. Allende Prieto⁵ and D. Kiselman⁶

¹ Research School of Astronomy and Astrophysics, Mt. Stromlo Observatory, Cotter Rd., Weston, ACT 2611, Australia e-mail: martin@mso.anu.edu.au
² Centre Spatial de Liège, Université de Liège, avenue Pré Aily, 4031 Angleur-Liège, Belgium
³ Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août, 17, B5C, 4000 Liège, Belgium
⁴ Observatoire Royal de Belgique, avenue circulaire, 3, 1180 Bruxelles, Belgium
⁵ McDonald Observatory and Department of Astronomy, University of Texas, Austin, TX 78712-1083, USA
⁶ The Institute for Solar Physics of the Royal Swedish Academy of Sciences, AlbaNova University Centre, 106 91 Stockholm, Sweden

This article has no abstract.

Key words: convection / line: formation / Sun: abundances / Sun: granulation / Sun: photosphere / errata, addenda

Erratum to: A&A, 417, 751–768 (2004), DOI: 10.1051/0004-6361:20034328

© ESO, 2005

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