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Correction to: The puzzling high velocity G5 supergiant star HD 179821: new insight from Gaia DR2 data

  • M. ParthasarathyEmail author
  • G. Jasniewicz
  • F. Thěvenin
Correction
  • 49 Downloads

Correction to: Astrophys Space Sci   https://doi.org/10.1007/s10509-019-3506-3

Unfortunately the original publication is missing Fig. 1. Please find the figure here:
Fig. 1

HR diagram. HD 179821 is located with \(T_{\mathrm{eff}} = 5660\) K and \(\log(L/L_{\odot}) = 4.3 \pm 0.2\) (see Sect. 3). The post-AGB models come from Miller Bertolami (2016); the initial masses and metallicities are indicated

Notes

References

  1. Miller Bertolami, M.M.: Astron. Astrophys. 588, A25 (2016) ADSCrossRefGoogle Scholar

Copyright information

© Springer Nature B.V. 2019

Authors and Affiliations

  1. 1.Indian Institute of AstrophysicsBangaloreIndia
  2. 2.UMR 5299 LUPM CNRS/Universitè MontpellierMontpellier cedex 05France
  3. 3.Observatoire de la Côte d’AzurUMR 6202 Cassiopée/CNRSNice cedex 4France

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