Purveyors of fine halos - II. Chemodynamical association of halo stars with Milky Way globular clusters

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Volume 637 (May 2020)

A&A, 637 (2020) A98

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Table C.1.

Candidate cluster escapees in the near-field of clusters (method I).

Gaia DR2 source ID	α^(a)	δ^(a)	r/r_t	ϖ	μ_α cos δ	μ_δ	v_r	[Fe/H]	P(A/B)	G	G_BP − G_RP
	[deg]	[deg]		[mas]	[mas yr⁻¹]	[mas yr⁻¹]	[km s⁻¹]	[dex]		[mag]	[mag]
NGC 4147
3950157700750904064	182.459	18.773	2.4	0.06 ± 0.15	−1.9 ± 0.2	−2.1 ± 0.2	184.8 ± 5.7	−1.53 ± 0.16	0.87	17.69	1.01
3950527823852135808	183.537	19.185	11.4	−0.57 ± 0.38	−3.8 ± 1.0	−1.7 ± 0.4	188.1 ± 10.9	−1.90 ± 0.17	0.06	19.22	0.77
3950992882911234944	182.416	19.691	11.4	−0.48 ± 0.46	−3.2 ± 0.9	−1.7 ± 0.4	160.6 ± 10.5	−1.91 ± 0.15	0.05	19.41	0.72

Notes. Only a small portion of the data is shown to indicate the form and content of the table.

^(a)

Coordinates are in the Gaia DR2 reference epoch J2015.5.

^(b)

Remarks: (1): Classified as being a CN-strong giant in Paper I. (2): Identified as RR Lyrae star. The full table is available through the CDS.

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