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Erratum
This article is an erratum for: [this article]

Issue
A&A
Volume 508, Number 1, December II 2009
Page(s) 209 - 210
Section Extragalactic astronomy
DOI https://doi.org/10.1051/0004-6361/200912350e
Published online 26 November 2009

A&A 508, 209-210 (2009)

Probing X-ray irradiation in the nucleus of NGC 1068 with observations of high-J lines of dense gas tracers  

(Erratum)

J. P. Pérez-Beaupuits1 - M. Spaans1 - F. F. S. van der Tak2,1 - S. Aalto3 - S. García-Burillo4 - A. Fuente4 - A. Usero4


1 - Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands
2 - SRON Netherlands Institute for Space research, Landleven 12, 9747 AD Groningen, The Netherlands
3 - Onsala Rymdobservatorium, Chalmers Tekniska Högskola, 439 92 Onsala, Sweden
4 - Observatorio Astronómico Nacional, C/ Alfonso XII 3, 28014 Madrid, Spain

A&A 503, 459-466 (2009), DOI: 10.1051/0004-6361/200912350


Key words: galaxies: ISM - galaxies: individual: NGC 1068 - galaxies: Seyfert - ISM: molecules: - radio lines: ISM - radio lines: galaxies - errata, addenda

An error occurred during the final processing of the publication of Fig. 1. The first spectrum of Fig. 1 has been published four times, replacing the three other spectra. The correct Fig. 1 is published on the next page.

\begin{figure}
\par\includegraphics[angle=-90,width=6cm,clip]{12350f01.ps}\\
\...
...ce*{2mm}
\includegraphics[angle=-90,width=6cm,clip]{12350f05.ps}
\end{figure} Figure 1:

Molecular line emissions in NGC 1068. The velocity resolution was reduced to 20  ${\rm km~s}^{-1}$ for all the lines. The spectra are centered with respect to the heliocentric systemic velocity $v_{\rm sys} = 1137$  ${\rm km~s}^{-1}$.

Open with DEXTER

  \begin{figure}
\par\includegraphics[angle=-90,width=6cm,clip]{12350f01.ps}\\
\...
...ce*{2mm}
\includegraphics[angle=-90,width=6cm,clip]{12350f05.ps}
\end{figure} Figure 1:

Molecular line emissions in NGC 1068. The velocity resolution was reduced to 20  ${\rm km~s}^{-1}$ for all the lines. The spectra are centered with respect to the heliocentric systemic velocity $v_{\rm sys} = 1137$  ${\rm km~s}^{-1}$.

Open with DEXTER In the text
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Copyright ESO 2009

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