Prospects for galactic and stellar astrophysics with asteroseismology of giant stars in the tess continuous viewing zones and beyond

HIGHLIGHTS

• who: MNRAS from the In particular, this paper has demonstrated the great importance of spectroscopic follow up for giants in the TESS-CVZsWe predict that seismic samples of the order of a few , giants could be attainable in the CVZs, but age and mass estimates will only be readily available, and sufficiently precise, for stars that also have spectroscopic information. Such spectroscopic data will likely become available from future survey data (e_g GALAH: Martell et_al , have published the research work: Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the TESS continuous viewing zones . . .
  

   

  

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