Pismis 7
(VDBH 43; MWSC 1532; OCL 734; vdBergh-Hagen 43; ESO 313 09; FSR 1393)
0.90
UTI
0.77
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.9 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Pismis 7 is a rich, very dense 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 massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Distant
Moderate extinction
Massive
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 | 130.282 | -38.7 | 0.167 | -3.284 | 2.823 | 73.384 |
| Li et al. | 2025 | 130.287 | -38.699 | 0.15 | -3.312 | 2.793 | â |
| Hu & Soubiran | 2025 | 130.295 | -38.698 | â | â | â | â |
| Almeida et al. | 2025 | 130.287 | -38.696 | â | â | â | â |
| Hunt & Reffert | 2024 | 130.28 | -38.703 | 0.165 | -3.271 | 2.828 | 71.574 |
| Cavallo et al. | 2024 | 130.295 | -38.698 | 0.172 | â | â | â |
| Hunt & Reffert | 2023 | 130.28 | -38.703 | 0.165 | -3.271 | 2.828 | 71.574 |
| Just et al. | 2023 | 130.295 | -38.704 | â | â | â | â |
| Jaehnig et al. | 2021 | 130.291 | -38.695 | 0.18 | -3.319 | 2.783 | â |
| Rain et al. | 2021 | 130.287 | -38.699 | 0.15 | -3.312 | 2.793 | â |
| Dias et al. | 2021 | 130.287 | -38.696 | 0.15 | -3.307 | 2.789 | 74.721 |
| Cantat-Gaudin et al. | 2020 | 130.287 | -38.699 | 0.15 | -3.312 | 2.793 | â |
| Cantat-Gaudin & Anders | 2020 | 130.287 | -38.699 | 0.15 | -3.312 | 2.793 | â |
| Soubiran et al. | 2018 | 130.287 | -38.699 | â | â | â | 74.4 |
| Bica et al. | 2019 | 130.277 | -38.701 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 130.287 | -38.699 | 0.15 | -3.312 | 2.793 | â |
| Kharchenko et al. | 2016 | 130.295 | -38.704 | â | â | â | â |
| Kharchenko et al. | 2013 | 130.3 | -38.707 | â | -3.54 | 8.67 | â |
| Dias et al. | 2002 | 130.283 | -38.7 | â | -0.23 | 2.86 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 4.79 | 2.07 | â | 597 | 0.166 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.150* | â | â | â |
| Almeida et al. | 2025 | 3.84 | 2.08 | â | 929 | â | 1014 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2361* | â | â |
| Cavallo et al. | 2024 | 4.00 | 2.29 | â | 776 | -0.280 | â | â | â |
| Hunt & Reffert | 2023 | 5.20 | 2.35 | 1.56 | 307 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 507 | â | 1387 | â | â |
| Jaehnig et al. | 2021 | 5.47* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 5.57 | 2.14 | â | 501 | â | â | â | 0 |
| Dias et al. | 2021 | 3.84 | 2.08 | â | 929 | -0.225 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.61 | 1.60 | â | 776 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.57 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.57 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.57 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.78 | 2.90 | â | 507 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.78 | 2.90 | â | 507 | â | â | â | â |
| Dias et al. | 2002 | 4.90 | 2.14 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.