Arp Madore 2
(Arp-Mado. 2; MWSC 1294; AM 2; ESO 368 07)
0.63
UTI
0.76
CN
0.5
Cdens
0.62
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
2.5 [N/pc2]
- CN 0.76 Rich
- Cdens 0.5 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
Arp Madore 2 is a rich, moderately dense object of intermediate C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an extremely massive, near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 114.686 | -33.845 | 0.065 | -0.528 | 1.263 | 125.142 |
| Just et al. | 2023 | 114.671 | -33.833 | â | â | â | â |
| Perren et al. | 2022 | 114.683 | -33.845 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 114.683 | -33.845 | 0.039 | -0.513 | 1.225 | â |
| Cantat-Gaudin & Anders | 2020 | 114.683 | -33.845 | 0.039 | -0.513 | 1.225 | â |
| Bica et al. | 2019 | 114.685 | -33.84 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 114.683 | -33.845 | 0.039 | -0.513 | 1.225 | â |
| Kharchenko et al. | 2016 | 114.671 | -33.833 | â | â | â | â |
| Dias et al. | 2014 | 114.692 | -33.843 | â | -3.51 | 1.63 | â |
| Kharchenko et al. | 2013 | 114.676 | -33.835 | â | 0.52 | 7.96 | â |
| van den Bergh | 2006 | 114.692 | -33.843 | â | â | â | â |
| Dias et al. | 2002 | 114.692 | -33.843 | â | 0.52 | 7.96 | 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 | 13.34 | 1.77 | â | 2163 | -0.330 | 12556 | 0.34 | â |
| Just et al. | 2023 | â | â | â | 2163 | â | 15311 | â | â |
| Perren et al. | 2022 | 10.91 | 1.95 | â | 4074 | -0.330 | 9800 | 0.34 | â |
| Cantat-Gaudin et al. | 2020 | 11.75 | 1.49 | â | 3020 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 14.62 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 14.62 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 13.34 | 1.77 | â | 2163 | â | â | â | â |
| Kharchenko et al. | 2013 | 13.34 | 1.77 | â | 2163 | â | â | â | â |
| van den Bergh | 2006 | 13.34 | 1.77 | â | 2188 | â | â | â | â |
| Dias et al. | 2002 | 13.34 | 1.77 | â | 2163 | â | â | â | â |
MOCA

