Volume 592, August 2016
|Number of page(s)||1|
|Section||Galactic structure, stellar clusters and populations|
|Published online||02 August 2016|
Equivalence of Boltzmann and moment equations (Corrigendum)
Dept. de Matemàtiques, Universitat Politècnica de Catalunya, 08034 Barcelona, Spain
Key words: stars: kinematics and dynamics / Galaxy: kinematics and dynamics / galaxies: statistics / methods: analytical / hydrodynamics / errata, addenda
In Cubarsi (2010)’s Eq. (15) relating the symmetric tensor components Λi1...ik and λi1i2...ik was not correctly written. It should be where means the symmetrized tensor.
They are now symmetric quantities, all the results remain totally valid.
- Cubarsi, R. 2010, A&A, 522, A30 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© ESO, 2016
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