| Issue |
A&A
Volume 618, October 2018
|
|
|---|---|---|
| Article Number | C6 | |
| Number of page(s) | 1 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361/201730725e | |
| Published online | 16 October 2018 | |
Corrigendum
The discrepancy between dynamical and theoretical mass in the triplet-system 2MASS J10364483+1521394 (Corrigendum)
1
Department of Astronomy, Stockholm University,
Stockholm,
Sweden
e-mail: per.calissendorff@astro.su.se
2
Institut für Astro- und Teilchenphysik, Universität Innsbruck,
Technikerstr. 25/8,
6020
Innsbruck,
Austria
3
Department of Astrophysics, University of Vienna,
Vienna,
Austria
4
Astrophysics Research Centre, Queens University, Belfast,
UK
5
Max Planck Institute for Astronomy,
Heidelberg,
Germany
6
NASA Goddard Space Flight Center,
Greenbelt,
MD
20771,
USA
An arithmetic error was made in the calculations of the optimal distance where the theoretical mass and dynamical mass would coincide. The updated estimation of the optimal distance is 17.2 ± 0.2 pc, corresponding to both theoretical and dynamical masses of ≈0.15 M⊙ for the B and C components individually. These updated values only change the numbers in the discussion of the optimal distance and do not change the main results of the paper.
© ESO 2018
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