Waterloo 7
(MWSC 1220)
0.85
UTI
0.51
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.51 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Waterloo 7 is a moderately populated, very 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 and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Distant
Moderate extinction
Near-solar metallicity
Young
Contains BSS
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 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 |
| 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 |
| 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| 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 | β | β | β | β | β | 503* | 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 | 1.27 | 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 |
| Cantat-Gaudin & Anders | 2020 | 3.35 | β | β | β | β | β | β | β |
| Monteiro & Dias | 2019 | 3.73 | 1.30 | 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 | 0.57 | β | 93 | β | β | β | β |
| Kharchenko et al. | 2016 | 2.93 | 1.10 | β | 339 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.93 | 1.10 | β | 339 | β | β | β | β |
| van den Bergh | 2006 | 2.80 | 1.30 | β | β | β | β | β | β |
| Dias et al. | 2002 | 2.80 | 1.30 | β | β | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.