Table B.6.
Considered GGCs.
Name | In-situ/Accr. | Oo Type | Prog. | NRRL | RA | Dec | d | μRA | μDec | RV |
---|---|---|---|---|---|---|---|---|---|---|
[deg] | [deg] | [kpc] | [mas/yr] | [mas/yr] | [km/s] | |||||
NGC104 | 1 | 0 | M-D | 48 | 6.024 | -72.081 | 4.52 ± 0.03 | 5.252 ± 0.021 | -2.551 ± 0.021 | -17.44 ± 0.16 |
NGC1261 | 0 | 1 | G-E | 9 | 48.068 | -55.216 | 16.40 ± 0.19 | 1.596 ± 0.025 | -2.064 ± 0.025 | 71.34 ± 0.21 |
NGC1851 | 0 | 1 | G-E | 21 | 78.528 | -40.047 | 11.95 ± 0.13 | 2.145 ± 0.024 | -0.65 ± 0.024 | 321.39 ± 1.55 |
NGC1904 | 0 | 2 | H99 | 5 | 81.044 | -24.524 | 13.08 ± 0.18 | 2.469 ± 0.025 | -1.594 ± 0.025 | 205.75 ± 0.2 |
NGC2298 | 0 | 0 | G-E | 9 | 102.248 | -36.005 | 9.83 ± 0.17 | 3.32 ± 0.025 | -2.175 ± 0.026 | 147.15 ± 0.57 |
Notes. Name of the GGC; classification of GGCs according to Belokurov & Kravtsov (2024): in situ = 1 accreted = 0; classification of GGCs according to Callingham et al. (2022), meaning of the acronyms is provided in Table B.5; Oo type lists the classification of GGCs in Oosterhoff types according to van den Bergh (2011) and Stobie (1971): 0, 1 and 2 refer to no-classification, OoI and OoII, respectively; NRRL is the number of RRLs for each GGCs collected from Clement et al. (2001); RA, Dec, d, μRA, μDec and RV are equatorial coordinates (J2000), distances, proper motions and radial velocities of the GGCs with relative errors according to the B&Co catalogue. Note that the GGC Mercer5 was not classified by Belokurov & Kravtsov (2024). We classified this GGC as in situ based on its position in the (E, Lz) diagram. Only a portion of the table is shown here to guide the reader about its content. A machine-readable version of the full table is published at the CDS (Centre de Données astronomiques de Strasbourg, https://cds.u-strasbg.fr/)
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