Dissecting the AGB star L2 Puppis: a torus in the making (Corrigendum)⋆
1 Institut für Astrophysik, Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
e-mail: foteini.lykou@univie.ac.at
2 Institut d’Astronomie et d’Astrophysique, Université Libre de Bruxelles, CP 226, Boulevard du Triomphe, 1050 Bruxelles, Belgium
3 Jodrell Bank Centre of Astrophysics, Alan Turing Building, University of Manchester, Oxford Road, M13 9PL, Manchester, UK
4 UJF-Grenoble 1/CNRS-INSU, Institut de Planétologie et d’Astrophysique de Grenoble (IPAG), UMR, 5274 Grenoble, France
5 Sydney Institute for Astronomy, University of Sydney, 44 Rosehill St, Redfern, NSW 2016, Sydney, Australia
6 Department of Astronomy, Uppsala Universitet, Box 516, 75120 Uppsala, Sweden
7 Department of Astronomy, Cornell University, 222 Space Sciences Building, Ithaca, NY 14853-6801, USA
8 Laboratoire Lagrange, UMR 7293, Université de Nice-Sophia Antipolis, CNRS, Observatoire de la Côte d’Azur, Bd de l’Observatoire, BP 4229, 06304 Nice Cedex 4, France
9 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
10 Onsala Space Observatory, Department of Earth and Space Sciences, Chalmers University of Technology, 439-92 Onsala, Sweden
Key words: techniques: high angular resolution / methods: observational / stars: AGB and post-AGB / circumstellar matter / stars: evolution / errata, addenda
It has come to our attention that further clarification is needed with respect to Fig. 2 and Sect. 3.1 in the original published version of this article (Lykou et al. 2015). The correction is related to a citation made in Sect. 3.1 to the work of Meisner (2008) and the method used to derive the angular sizes presented in Fig. 2, which may confuse the reader. Our results, as presented in Fig. 2 and Sect. 3.1, were derived with a method independent of the one of Meisner (2008). The citation should be modified to J. Meisner (priv. comm.). This clarification does not modify the overall direction of our work.
Acknowledgments
We thank Dr. Jeff Meisner for pointing out this inconsistency, for many fruitful discussions on optical interferometry and for providing the reduced VINCI visibilities.
References
- Lykou, F., Klotz, D., Paladini, C., et al. 2015, A&A, 576, A46 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Meisner, J. 2008, in The Power of Optical/IR Interferometry: Recent Scientific Results and 2nd Generation, eds. A. Richichi, F. Delplancke, F. Paresce, & A. Chelli, 481 [Google Scholar]
© ESO, 2015