The second and third parameters of the horizontal branch in globular clusters

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Table 1:

Basic parameters for globular clusters considered in this paper ( $M_{\rm TO}$ and $M_{\rm RGB}$ are in solar masses).
Cluster	Other	[Fe/H]	(m-M)_V	E(B-V)	$M_{\rm V}$	HBR	Age	$M_{\rm TO}$	$M_{\rm RGB}$	IQR $_{\rm [Na/O]}$	IQR $_{\rm [Al/Mg]}$	$\log{T_{\rm eff}^{\rm max}}$ (HB)
		dex	mag	mag	mag			$M_\odot$	$M_\odot$	dex	dex	K
NGC 104	47 Tuc	-0.76	13.37	0.04	-9.42	-0.99	0.95	0.862	0.909	0.472	0.091	3.756
NGC 288		-1.32	14.83	0.03	-6.74	0.98	0.90	0.827	0.869	0.776	0.059	4.221
NGC 362		-1.30	14.81	0.03	-8.41	-0.87	0.80	0.858	0.900	0.670		4.079
IC 1257		-1.73	19.25	0.73	-6.15	-0.71
NGC 1261		-1.27	16.10	0.01	-7.81	1.00	0.79	0.847	0.887			4.079

Notes. The complete table is available at the CDS.

Source LaTeX | All tables | In the text

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