| Issue |
A&A
Volume 557, September 2013
|
|
|---|---|---|
| Article Number | C2 | |
| Number of page(s) | 2 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201218944e | |
| Published online | 04 September 2013 | |
Formation and evolution of dwarf early-type galaxies in the Virgo cluster
II. Kinematic scaling relations (Corrigendum)
1
Departamento de Astrofísica y CC. de la AtmósferaUniversidad Complutense de
Madrid,
28040
Madrid,
Spain
e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
, This email address is being protected from spambots. You need JavaScript enabled to view it.
2
UCO/Lick Observatory, University of California, Santa Cruz, 1156 High
Street, Santa Cruz,
CA
95064,
USA
3
Observatories of the Carnegie Institution of Washington, 813 Santa Barbara
Street, Pasadena,
CA
91101,
USA
4
Laboratoire d’Astrophysique de Marseille-LAM, Université
d’Aix-Marseille & CNRS, UMR 7326, 38 rue F. Joliot-Curie, 13388
Marseille Cedex 13,
France
e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
5
Kapteyn Astronomical Institute, Postbus 800, 9700 AV
Groningen, The
Netherlands
e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
6
Instituto de Astrofísica de Canarias, Vía Láctea s/n,
La Laguna, Tenerife, Spain
7
Departamento de Astrofísica, Universidad de La
Laguna, 38205, La
Laguna, Tenerife,
Spain
e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
8
Max Planck Institute for Astronomy, Kӧnigstuhl
17, 69117
Heidelberg,
Germany
e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
Key words: galaxies: clusters: individual: Virgo / galaxies: dwarf / galaxies: elliptical and lenticular, cD / galaxies: evolution / galaxies: kinematics and dynamics / errata, addenda
Fulbright Postdoctoral Fellow.
In the published article, Table 2 showed incorrect absolute magnitudes in the K band for 10 of the objects. This error only affected Col. 6 of that table and the middle panel of Fig. 1. The correct table and figure are included below. The conclusions of the published article are not affected whatsoever by this mistake.
Photometric parameters for the sample of dEs.
 |
Fig. 1 Comparison between the apparent magnitudes in our work and different sources from the literature. |
© ESO, 2013
All Tables
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