Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs (Corrigendum)

E. Papastergis; A. A. Ponomareva

doi:10.1051/0004-6361/201629546e

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Erratum

This article is an erratum for: [this article]

Issue		A&A Volume 603, July 2017


Article Number		C4
Number of page(s)		1
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/201629546e
Published online		24 July 2017

A&A 603, C4 (2017)

Testing core creation in hydrodynamical simulations using the HI kinematics of field dwarfs (Corrigendum)

E. Papastergis¹ and A. A. Ponomareva²^,1

¹ Kapteyn Astronomical Institute, University of Groningen, Landleven 12, 9747 AD Groningen, The Netherlands
e-mail: papastergis@astro.rug.nl; ponomareva@astro.rug.nl
² Research School of Astronomy & Astrophysics, Australian National University, Canberra, ACT 2611, Australia

This article has no abstract.

Key words: galaxies: kinematics and dynamics / dark matter / galaxies: dwarf / galaxies: halos / radio lines: galaxies / errata, addenda

Erratum to: A&A 601, A1 (2017), DOI: 10.1051/0004-6361/201629546

© ESO, 2017

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