Waterloo 3
(MWSC 1381)
0.58
UTI
0.47
CN
0.46
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.47 Poorly populated
- Cdens 0.46 Loose
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Waterloo 3 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Very distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 118.775 | -25.356 | 0.193 | -2.365 | 2.685 | 91.877 |
| Hunt & Reffert | 2024 | 118.778 | -25.358 | 0.197 | -2.408 | 2.671 | 116.962 |
| Cavallo et al. | 2024 | 118.818 | -25.422 | 0.196 | â | â | â |
| Hunt & Reffert | 2023 | 118.778 | -25.358 | 0.197 | -2.408 | 2.671 | 116.962 |
| Just et al. | 2023 | 118.761 | -25.369 | â | â | â | â |
| Monteiro & Dias | 2019 | 118.775 | -25.365 | â | -2.331 | 2.67 | 2.232 |
| Kharchenko et al. | 2016 | 118.761 | -25.369 | â | â | â | â |
| Dias et al. | 2014 | 118.775 | -25.365 | â | -2.11 | 2.83 | â |
| Kharchenko et al. | 2013 | 118.767 | -25.372 | â | -1.18 | 3.41 | â |
| van den Bergh | 2006 | 118.775 | -25.365 | â | â | â | â |
| Dias et al. | 2002 | 118.775 | -25.365 | â | -1.18 | 3.41 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 356* | â | â |
| Cavallo et al. | 2024 | 3.61 | 0.76 | â | 309 | -0.200 | â | â | â |
| Hunt & Reffert | 2023 | 5.11 | 0.43 | 1.35 | 282 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 316 | â | 224 | â | â |
| Monteiro & Dias | 2019 | 7.96 | 1.40 | â | 10 | 0.036 | â | â | â |
| Kharchenko et al. | 2016 | 2.59 | 1.29 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.59 | 1.29 | â | 316 | â | â | â | â |
| van den Bergh | 2006 | 5.20 | 1.05 | â | â | â | â | â | â |
| Dias et al. | 2002 | 5.20 | 1.05 | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.