| Issue |
A&A
Volume 583, November 2015
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201527565 | |
| Published online | 29 October 2015 | |
Surface brightness profile of the Milky Way’s nuclear star cluster (Corrigendum)
1
Instituto de Astrofísica de Andalucía (CSIC),
Glorieta de la Astronomía s/n,
18008
Granada,
Spain
e-mail:
rainer@iaa.es
2
European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748
Garching bei München,
Germany
3
Astronomical Institute, Academy of Sciences,
Boční II 1401, 14100
Prague, Czech
Republic
4
El Camino College, 16007 Crenshaw Blvd.,
Torrance, CA
90506,
USA
5
Max-Planck Institut für Gravitationsphysik
(Albert-Einstein-Institut), Am
Mühlenberg 1, 14476
Potsdam,
Germany
6
National Astronomical Observatory of Japan,
Mitaka, 181-8588
Tokyo,
Japan
Key words: dust, extinction / Galaxy: center / Galaxy: nucleus / Galaxy: structure / galaxies: nuclei / errata, addenda
In Schödel et al. (2014), the axis labels of Figs. 4, 6−9, 11, and 13 should not refer to “RA” (Right ascension) and “Dec” (Declination) because the orientation of all the images is such that Galactic north is up and Galactic east is to the left. Instead, the axis labels indicate the offsets from Sagittarius A* parallel and perpendicular to the Galactic plane, as is correctly described in Fig. 1 and its caption.
Acknowledgments
We thank Ortwin Gerhard for bringing this to our attention.
References
- Schödel, R., Feldmeier, A., Kunneriath, D., et al. 2014, A&A, 566, A47 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2015
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