Arches
(BDB2003 G000.12+00.01)
0.16
UTI
0.65
CN
0.13
Cdens
0.12
CC3
0.0
Clit
0.88
Cdup
Nm (P>50%)
80
Core radius and density
1.0 [pc], 0.6 [pc-2]
- CN 0.65 Moderately populated
- Cdens 0.13 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.88 Very likely unique
Overview
Arches is a moderately populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.
(*): The parallax distance estimate (~2.05 kpc) differs significantly from the median photometric distance (~8.23 kpc).
Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.88) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 266.517 | -28.848 | 0.489 | 0.075 | -2.101 | 21.145 |
| Morales et al. | 2013 | 266.458 | -28.823 | â | â | â | â |
| Bica et al. | 2003 | 266.467 | -28.829 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 8.23 | â | â | 2 | â | â | â | â |
| Morales et al. | 2013 | 8.23 | â | â | 2 | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded.
Bica et al. (2003)
Classified as infrared cluster (IRC).