Absolute dimensions of eclipsing binaries - XXVIII. BK Pegasi and other F-type binaries: Prospects for calibration of convective core overshoot

J. V. Clausen; S. Frandsen; H. Bruntt; E. H. Olsen; B. E. Helt; K. Gregersen; D. Juncher; P. Krogstrup

doi:10.1051/0004-6361/201014266

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Volume 516 (June-July 2010)

A&A, 516 (2010) A42

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Table 4:

Radial velocities of BK Peg and residuals from the final spectroscopic orbit presented in Table 8.
HJD	Phase	$RV_{\rm p}$	$RV_{\rm s}$	$({\rm O-C})_{\rm p}$	$({\rm O-C})_{\rm s}$
-2 400 000		kms^-1	kms^-1	kms^-1	kms^-1
54333.45954	0.6647	60.398	-83.802	0.25	0.28
54333.46395	0.6655	60.694	-83.936	0.35	0.38
54334.42028	0.8397	58.578	-81.562	-0.50	0.09
54335.52799	0.0414	-28.144	15.916	-0.19	-0.38
54335.53872	0.0434	-28.875	16.995	0.02	-0.33
54335.62203	0.0586	-36.037	24.823	0.05	-0.42
54335.72881	0.0780	-44.698	34.832	0.22	-0.10
54336.41869	0.2037	-83.237	77.803	0.15	0.44
54336.43503	0.2067	-83.671	78.279	0.11	0.47
54336.52436	0.2229	-85.447	80.223	0.03	0.45
54336.74168	0.2625	-86.151	81.269	-0.01	0.50
54337.44772	0.3911	-56.696	48.134	-0.20	-0.59
54337.58944	0.4169	-46.161	36.119	-0.28	-0.80

Source LaTeX | All tables | In the text

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