Pismis 8
(MWSC 1533; FoF 2088)
0.95
UTI
0.74
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
10.7 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Pismis 8 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below 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 absorption and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with 3 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 130.391 | -46.274 | 0.537 | -5.713 | 4.986 | â |
| Almeida et al. | 2025 | 130.409 | -46.271 | â | â | â | â |
| Hunt & Reffert | 2024 | 130.404 | -46.263 | 0.533 | -5.672 | 4.981 | â |
| Cavallo et al. | 2024 | 130.408 | -46.267 | 0.533 | â | â | â |
| Hunt & Reffert | 2023 | 130.404 | -46.263 | 0.533 | -5.672 | 4.981 | â |
| Almeida et al. | 2023 | 130.413 | -46.272 | â | â | â | â |
| Just et al. | 2023 | 130.41 | -46.264 | â | â | â | â |
| Jaehnig et al. | 2021 | 130.398 | -46.275 | 0.554 | -5.743 | 4.973 | â |
| Rain et al. | 2021 | 130.407 | -46.272 | 0.517 | -5.757 | 4.945 | â |
| Richer et al. | 2021 | 130.406 | -46.269 | 0.521 | -5.698 | 4.926 | â |
| Dias et al. | 2021 | 130.409 | -46.271 | 0.514 | -5.726 | 4.912 | â |
| Cantat-Gaudin et al. | 2020 | 130.407 | -46.272 | 0.517 | -5.757 | 4.945 | â |
| Cantat-Gaudin & Anders | 2020 | 130.407 | -46.272 | 0.517 | -5.757 | 4.945 | â |
| Liu & Pang | 2019 | 130.435 | -46.288 | 0.506 | -5.72 | 4.895 | â |
| Cantat-Gaudin et al. | 2018 | 130.407 | -46.272 | 0.517 | -5.757 | 4.945 | â |
| Loktin & Popova | 2017 | 130.395 | -46.266 | â | -3.29 | 3.07 | 63.4 |
| Kharchenko et al. | 2016 | 130.41 | -46.264 | â | â | â | â |
| Dias et al. | 2014 | 130.4 | -46.267 | â | â | â | 63.4 |
| Kharchenko et al. | 2013 | 130.414 | -46.267 | â | -4.97 | 9.43 | â |
| Bukowiecki et al. | 2011 | 130.4 | -46.276 | â | â | â | â |
| van den Bergh | 2006 | 130.396 | -46.273 | â | â | â | â |
| Dias et al. | 2002 | 130.4 | -46.267 | â | -3.29 | 3.07 | 63.4 |
| Dambis | 1999 | 130.396 | -46.273 | â | â | â | 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 | 1.78 | 2.19 | 1.1 | 27 | 0.088 | 250 | 0.62 | 0.0 |
| Liu et al. | 2025 | 2.98 | 0.69 | â | 22 | â | â | â | â |
| Almeida et al. | 2025 | 1.76 | 2.08 | â | 14 | â | 262 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 219(1) | â | â |
| Cavallo et al. | 2024 | 1.92 | 2.45 | â | 31 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 1.89 | 2.16 | 1.10 | 47 | â | â | â | â |
| Almeida et al. | 2023 | 1.75 | 2.23 | â | 14 | -0.037 | 250(1) | 0.62 | â |
| Just et al. | 2023 | â | â | â | 27 | â | 12 | â | â |
| Jaehnig et al. | 2021 | 1.80(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.83 | 2.17 | â | 26 | â | â | â | 0 |
| Richer et al. | 2021 | â | 2.42 | â | â | â | â | â | â |
| Dias et al. | 2021 | 1.76 | 2.08 | â | 14 | -0.034 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.91 | 1.58 | â | 32 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.83 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 47 | 0.500 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.83 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.31 | 2.19 | â | 27 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.36 | 2.19 | â | 27 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.36 | 2.19 | â | 27 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 254 | â | â |
| Bukowiecki et al. | 2011 | 1.86(1) | 2.26 | â | 32 | â | â | â | â |
| van den Bergh | 2006 | 1.31 | 2.20 | â | 27 | â | â | â | â |
| Dias et al. | 2002 | 1.31 | 2.19 | â | 27 | â | â | â | â |
| Dambis | 1999 | 1.41 | 2.24 | â | 32 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 330 along with Pismis_6.
Palma et al. (2025)
Classified as genetic pair P164, along with Pismis_6.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit. Silver sample.