| Issue |
A&A
Volume 652, August 2021
|
|
|---|---|---|
| Article Number | C5 | |
| Number of page(s) | 1 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201628623e | |
| Published online | 13 August 2021 | |
Brown dwarf disks with ALMA: evidence for truncated dust disks in Ophiuchus (Corrigendum)
1
ESO/European Southern Observatory, Karl-Schwarzschild-Strasse 2,
85748
Garching bei München,
Germany
e-mail: ltesti@eso.org
2
Excellence Cluster “Universe”, Boltzmann str. 2,
85748
Garching bei Muenchen, Germany
3
INAF/Osservatorio Astrofisico of Arcetri, Largo E. Fermi, 5,
50125
Firenze,
Italy
4
Gothenburg Center for Advance Studies in Science and Technology, Department of Mathematical Sciences, Chalmers University of Technology and University of Gothenburg, 412 96
Gothenburg, Sweden
5
School of Cosmic Physics, Dublin Institute for Advanced Studies, 31 Fitzwilliams Place,
Dublin 2, Ireland
6
SUPA, School of Physics and Astronomy, University of St. Andrews, North Haugh, St. Andrews,
Fife
KY16 9SS, UK
7
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street,
Cambridge,
MA
02138,
USA
8
Joint ALMA Observatory (JAO), Alonso de Cordova 3107
Vitacura -Santiago de Chile, Chile
Key words: protoplanetary disks / brown dwarfs / stars: formation / submillimeter: planetary systems / errata, addenda
An error occurred in the paper: the object ISO-Oph 164 was not observed by ALMA as part of project 2012.1.00037.S. The object observed (see the ALMA image in Fig. 1) was instead GY92 317 (Greene & Young 1992). This object is probably a field star, as discussed in Barsony et al. (1997). The upper limit for the millimetre flux of ISO-Oph 164 reported in Table 2 is thus incorrect.
None of the conclusions of the paper is affected by this error.
References
- Barsony, M., Kenyon, S. J., Lada, E. A., & Teuben, P. J. 1997, ApJS, 112, 109 [NASA ADS] [CrossRef] [Google Scholar]
- Greene, T. P., & Young, E. T. 1992, ApJ, 395, 516 [NASA ADS] [CrossRef] [Google Scholar]
© ESO 2021
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