| Issue |
A&A
Volume 577, May 2015
|
|
|---|---|---|
| Article Number | C1 | |
| Number of page(s) | 1 | |
| Section | Galactic structure, stellar clusters and populations | |
| DOI | https://doi.org/10.1051/0004-6361/201423481e | |
| Published online | 28 April 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
The first column of Table 4 for the multi-Gaussian expansion (MGE) fits contains an error. The maximum intensity of the Gaussian components I is in 105L⊙ ,4.5 μm/ pc2 and not in 106L⊙ ,4.5 μm/ pc2. A correct version of the table is presented here.
MGE fit parameters for the Spitzer/IRAC PAH- and extinction-corrected image.
Acknowledgments
We thank Troy Raen for bringing this to our attention.
© ESO, 2015
All Tables
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