| 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
This article has no abstract.
Key words: dust, extinction / Galaxy: center / Galaxy: nucleus / Galaxy: structure / galaxies: nuclei / errata, addenda
© ESO, 2015
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.
