Issue |
A&A
Volume 668, December 2022
|
|
---|---|---|
Article Number | C2 | |
Number of page(s) | 1 | |
Section | Galactic structure, stellar clusters and populations | |
DOI | https://doi.org/10.1051/0004-6361/202038840e | |
Published online | 08 December 2022 |
Towards a fully consistent Milky Way disk model
IV. The impact of Gaia DR2 and APOGEE (Corrigendum)
Astronomisches Rechen-Institut, Zentrum für Astronomie der Universität Heidelberg, Mönchhofstr. 12–14, 69120 Heidelberg, Germany
e-mail: Sysoliatina@uni-heidelberg.de
Key words: Galaxy: disk / Galaxy: kinematics and dynamics / solar neighborhood / Galaxy: evolution / errata, addenda
We have identified several typographical errors in our paper. These typos did not affect our modelling, and all results presented in Sysoliatina & Just (2021) remain valid.
First, the star-formation rate (SFR) parameters ζ and η were by mistake interchanged in Eq. (11). The correct expression for the galactic time corresponding to the SFR maximum reads
Second, there was a minus sign missing in the second exponent of the second term of Eq. (17). The formula for the convolution of a linear cumulative metallicity distribution with aGaussian kernel should read
We give the correct version of this equation in our subsequent paper, Sysoliatina & Just (2022, Eq. (20)).
Finally, the last digit of our project ID was missing. The correct acknowledgement should be “This work was supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – Project-ID 138713538 – SFB 881 (‘The Milky Way System’, subproject A06)”.
References
- Sysoliatina, K., & Just, A. 2021, A&A, 647, A39 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
- Sysoliatina, K., & Just, A. 2022, A&A, 666, A130 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
© The Authors 2022
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