SIMBAD references

2012ApJ...751L..36W - Astrophys. J., 751, L36 (2012/June-1)

Solving the mode identification problem in asteroseismology of f stars observed with Kepler.

WHITE T.R., BEDDING T.R., GRUBERBAUER M., BENOMAR O., STELLO D., APPOURCHAUX T., CHAPLIN W.J., CHRISTENSEN-DALSGAARD J., ELSWORTH Y.P., GARCIA R.A., HEKKER S., HUBER D., KJELDSEN H., MOSSER B., KINEMUCHI K., MULLALLY F. and STILL M.

Abstract (from CDS):

Asteroseismology of F-type stars has been hindered by an ambiguity in identification of their oscillation modes. The regular mode pattern that makes this task trivial in cooler stars is masked by increased line widths. The absolute mode frequencies, encapsulated in the asteroseismic variable ε, can help solve this impasse because the values of ε implied by the two possible mode identifications are distinct. We find that the correct ε can be deduced from the effective temperature and the line widths and we apply these methods to a sample of solar-like oscillators observed with Kepler.

Abstract Copyright:

Journal keyword(s): stars: fundamental parameters - stars: interiors - stars: oscillations

Simbad objects: 59

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2019.10.17-13:57:55

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