Young giants of intermediate mass. Evidence of rotation and mixing

@article{Lombardo2021YoungGO,
  title={Young giants of intermediate mass. Evidence of rotation and mixing},
  author={Linda Lombardo and Patrick Franccois and Piercarlo Bonifacio and E. Caffau and A. M. Matas Pinto and Corinne Charbonnel and Georges Meynet and Lorenzo Monaco and Gabriele Cescutti and Alessio Mucciarelli},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. In the search of a sample of metal-poor bright giants using Strömgren photometry, we serendipitously found a sample of 26 young (ages younger than 1 Gyr) metal-rich giants, some of which have high rotational velocities. Aims. We determined the chemical composition and rotational velocities of these stars in order to compare them with predictions from stellar evolution models. These stars where of spectral type A to B when on the main sequence, and we therefore wished to compare their… 

References

SHOWING 1-6 OF 6 REFERENCES
in Modelling of Stellar Atmospheres
The disclosure relates to a method of bending elongated materials such as pipe by applying a compressive primary bending force to the material at locations on either end of the portion of the
Turbospectrum: Code for spectral synthesis
consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement
  • A&A,
  • 2012
institutions, in particular the institutions participating in the Gaia Multilateral Agreement
  • A&A,
  • 2012
& Sophie Team
  • Tenth Anniversary of 51 Peg-b: Status of and prospects for hot Jupiter studies
  • 2006
Turbospectrum : Code for spectral synthesis (Astrophysics Source
  • A&A,
  • 2006