Fundamental properties of Kepler and CoRoT targets – III. Tuning scaling relations using the first adiabatic exponent

So-called scaling relations based on oscillation frequencies have the potential to reveal the mass and radius of solar-like oscillating stars. In the derivation of these relations, it is assumed that the first adiabatic exponent at the surface ( $\Gamma _{\rm \negthinspace 1s}$ ) of such stars is co...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-10, Vol.462 (2), p.1577-1590
Hauptverfasser:	Yıldız, M., Çelik Orhan, Z., Kayhan, C.
Format:	Artikel
Sprache:	eng
Schlagworte:	Adiabatic flow Astronomy Constants Exponents Frequencies Oscillating Photometry Star & galaxy formation Stars Stellar oscillations Tuning
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