| 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}](/articles/aa/full_html/2009/46/aa12350-09e/img4.png)
|
Figure 1:
Molecular line emissions in NGC 1068.
The velocity resolution was reduced to 20
|
| Open with DEXTER | |
Molecular line emissions in NGC 1068.
The velocity resolution was reduced to 20
for all the lines.
The spectra are centered with
respect to the heliocentric systemic velocity
.
Copyright ESO 2009