Red-giant seismic properties analyzed with CoRoT | Astronomy & Astrophysics (A&A)

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Table 4:

Scaling with $\nu _{{\rm max}}$ .
$f(\nu_{{\rm max}})$	$\langle\Delta\nu\rangle$	$T_{{\rm eff}}$	R	$\nu_{{\rm c}}$
exponent	$\beta$	$\gamma$	$\delta$	$\alpha$
giants	0.75 $\pm$ 0.01	0.04 $\pm$ 0.01	-0.48 $\pm$ 0.01	1.00 $\pm$ 0.02
subgiants⁽¹⁾	0.71 $\pm$ 0.02	-0.02 $\pm$ 0.02	-0.58 $\pm$ 0.06	0.83 $\pm$ 0.10
	0.77 $\pm$ 0.01 $^{\star}$			0.97 $\pm$ 0.10
dwarfs⁽²⁾	0.76 $\pm$ 0.02	-0.18 $\pm$ 0.02	-0.64 $\pm$ 0.03	0.97 $\pm$ 0.04
	0.77 $\pm$ 0.01 $^{\star}$			0.99 $\pm$ 0.04

Notes. $^{(\star)}$ Value from Stello et al. (2009).

References. (1) Kallinger et al. (2010); Deheuvels et al. (2010); (2) Kallinger et al. (2010); Mosser et al. (2008); Teixeira et al. (2009); Mathur et al. (2010a); Gaulme et al. (2010); J. Ballot, private communication.

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