Waterloo 7
(MWSC 1220)
0.73
UTI
0.51
CN
0.86
Cdens
0.75
CC3
0.77
Clit
1.0
Cdup
Nm (P>50%)
52
Core radius and density
1.1 [pc], 4.3 [pc-2]
- CN 0.51 Moderately populated
- Cdens 0.86 Dense
- CC3 0.75 High quality
- Clit 0.77 Well-studied
- Cdup 1.0 Unique
Overview
Waterloo 7 is a moderately populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 111.537 | -15.093 | 0.275 | -1.529 | 1.724 | 62.438 |
| Li et al. | 2025 | 111.532 | -15.09 | 0.27 | -1.514 | 1.695 | β |
| Almeida et al. | 2025 | 111.532 | -15.088 | β | β | β | β |
| Hunt & Reffert | 2024 | 111.537 | -15.092 | 0.264 | -1.521 | 1.728 | 59.398 |
| Cavallo et al. | 2024 | 111.547 | -15.089 | 0.263 | β | β | β |
| Hunt & Reffert | 2023 | 111.537 | -15.092 | 0.264 | -1.521 | 1.728 | 59.398 |
| Just et al. | 2023 | 111.526 | -15.091 | β | β | β | β |
| Rain et al. | 2021 | 111.532 | -15.09 | 0.27 | -1.514 | 1.695 | β |
| Dias et al. | 2021 | 111.532 | -15.088 | 0.267 | -1.521 | 1.681 | β |
| Cantat-Gaudin et al. | 2020 | 111.532 | -15.09 | 0.27 | -1.514 | 1.695 | β |
| SΓ‘nchez et al. | 2020 | 111.533 | -15.093 | β | -1.875 | 1.684 | β |
| Cantat-Gaudin & Anders | 2020 | 111.532 | -15.09 | 0.27 | -1.514 | 1.695 | β |
| Monteiro & Dias | 2019 | 111.533 | -15.093 | β | -1.484 | 1.697 | 2.58 |
| Bossini et al. | 2019 | 111.532 | -15.09 | β | β | β | β |
| Soubiran et al. | 2018 | 111.532 | -15.09 | β | β | β | 65.91 |
| Bica et al. | 2019 | 111.541 | -15.09 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 111.532 | -15.09 | 0.27 | -1.514 | 1.695 | β |
| Loktin & Popova | 2017 | 111.54 | -15.091 | β | -2.705 | 0.737 | 83.0 |
| Sampedro et al. | 2017 | 111.533 | -15.093 | β | 0.46 | 2.28 | β |
| Kharchenko et al. | 2016 | 111.526 | -15.091 | β | β | β | β |
| Dias et al. | 2014 | 111.533 | -15.093 | β | 0.28 | 1.27 | β |
| Kharchenko et al. | 2013 | 111.532 | -15.093 | β | -1.79 | 2.63 | 83.0 |
| Bukowiecki et al. | 2011 | 111.529 | -15.097 | β | β | β | β |
| van den Bergh | 2006 | 111.533 | -15.093 | β | β | β | β |
| Dias et al. | 2002 | 111.533 | -15.093 | β | -1.79 | 2.63 | β |
π‘ 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 | 99999β | 3.265 | 1.29 | 0.95 | 73 | 0.025 | 368 | β | 1 |
| Li et al. | 2025 | 3.12 | 1.26 | β | 79 | 0.033 | β | β | β |
| Almeida et al. | 2025 | 2.84 | 1.41 | β | 67 | β | 201 | β | β |
| Hunt & Reffert | 2024 | 3.20 | 1.10 | 0.95 | 192 | β | 503(1) | β | β |
| Cavallo et al. | 2024 | 3.33 | 1.50 | β | 20 | 0.210 | β | β | β |
| Hunt & Reffert | 2023 | 3.20 | 1.10 | 0.95 | 192 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 339 | β | 2366 | β | β |
| Rain et al. | 2021 | 3.35 | 1.29 | β | 58 | β | β | β | 1 |
| Dias et al. | 2021 | 2.84 | 1.41 | β | 67 | -0.107 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.56 | 1.48 | β | 30 | β | β | β | β |
| Kounkel et al. | 2020 | 3.43 | 1.16 | β | 182 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.35 | β | β | β | β | β | β | β |
| Monteiro & Dias | 2019 | 3.73 | 1.32 | β | 58 | 0.025 | β | β | β |
| Bossini et al. | 2019 | 3.68 | 1.32 | β | 45 | 0.000 | β | β | β |
| Soubiran et al. | 2018 | 3.35 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.35 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 4.23 | 0.58 | β | 93 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.93 | 1.12 | β | 339 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.93 | 1.12 | β | 339 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 232 | β | β |
| Bukowiecki et al. | 2011 | 1.98(1) | 0.82 | β | 28 | β | β | β | β |
| van den Bergh | 2006 | 2.80 | 1.32 | β | β | β | β | β | β |
| Dias et al. | 2002 | 2.80 | 1.32 | β | β | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.4101, e_all=0.3035.
Rain et al. (2021)
This cluster was include in (Dias et al., 2002A&A...389..871D, Cat. B/ocl) however, parameters log(t)=7.76, Av=0.418, Z=0.025were taken from Monteiro & Dias (2019MNRAS.487.2385M).
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).