Pismis 11
(MWSC 1643)
0.51
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.74
Clit
0.64
Cdup
Nm (P>50%)
216
Core radius and density
1.2 [pc], 9.3 [pc-2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.74 Moderately studied
- Cdup 0.64 Likely unique
Overview
Pismis 11 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. 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 | 99999β | 138.974 | -50.004 | 0.367 | -5.337 | 3.983 | 61.198 |
| Almeida et al. | 2025 | 138.973 | -50.01 | β | β | β | β |
| Hunt & Reffert | 2024 | 138.973 | -50.007 | 0.372 | -5.336 | 4.012 | 91.648 |
| Celli et al. | 2024 | 138.971 | -50.017 | β | β | β | β |
| Cavallo et al. | 2024 | 139.003 | -49.972 | 0.37 | β | β | β |
| Hunt & Reffert | 2023 | 138.973 | -50.007 | 0.372 | -5.336 | 4.012 | 91.648 |
| Almeida et al. | 2023 | 138.967 | -50.008 | β | β | β | β |
| Just et al. | 2023 | 138.966 | -50.007 | β | β | β | β |
| Jaehnig et al. | 2021 | 138.969 | -50.006 | 0.379 | -5.372 | 3.902 | β |
| Rain et al. | 2021 | 138.974 | -50.006 | 0.335 | -5.397 | 3.926 | β |
| Dias et al. | 2021 | 138.973 | -50.01 | 0.329 | -5.386 | 3.915 | β |
| Cantat-Gaudin et al. | 2020 | 138.974 | -50.006 | 0.335 | -5.397 | 3.926 | β |
| SΓ‘nchez et al. | 2020 | 138.971 | -50.017 | β | -5.353 | 3.904 | β |
| Cantat-Gaudin & Anders | 2020 | 138.974 | -50.006 | 0.335 | -5.397 | 3.926 | β |
| Cantat-Gaudin et al. | 2018 | 138.974 | -50.006 | 0.335 | -5.397 | 3.926 | β |
| Dias et al. | 2018 | β | β | β | -5.27 | 2.91 | β |
| Sampedro et al. | 2017 | 138.971 | -50.017 | β | -1.18 | 6.0 | β |
| Kharchenko et al. | 2016 | 138.966 | -50.007 | β | β | β | β |
| Dias et al. | 2014 | 138.971 | -50.017 | β | -0.86 | 7.3 | β |
| Kharchenko et al. | 2013 | 138.97 | -50.01 | β | 0.55 | 14.77 | -16.3 |
| Bukowiecki et al. | 2011 | 139.125 | -49.715 | β | β | β | β |
| Ahumada & Lapasset | 2007 | 139.175 | -49.717 | β | β | β | β |
| van den Bergh | 2006 | 138.95 | -50.017 | β | β | β | β |
| Dias et al. | 2002 | 138.971 | -50.017 | β | 0.55 | 14.77 | β |
| Lynga | 1987 | 139.177 | -49.712 | β | β | β | 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 | 2.75 | 3.79 | 2.79 | 6 | 0.051 | 467 | 0.81 | 0 |
| Almeida et al. | 2025 | 2.34 | 3.30 | β | 6 | β | 402 | β | β |
| Hunt & Reffert | 2024 | 2.49 | 4.18 | 2.79 | 7 | β | 2708(1) | β | β |
| Celli et al. | 2024 | β | β | β | 3 | β | 590 | β | β |
| Cavallo et al. | 2024 | 2.86 | 3.79 | β | 9 | 0.560 | β | β | β |
| Hunt & Reffert | 2023 | 2.49 | 4.18 | 2.79 | 7 | β | β | β | β |
| Almeida et al. | 2023 | 2.21 | 3.41 | β | 7 | 0.006 | 467(1) | 0.81 | β |
| Just et al. | 2023 | β | β | β | 1 | β | 169 | β | β |
| Jaehnig et al. | 2021 | 2.67(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.75 | 3.79 | β | 10 | β | β | β | 0 |
| Dias et al. | 2021 | 2.34 | 3.30 | β | 6 | 0.051 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.81 | 3.70 | β | 3 | β | β | β | β |
| Kounkel et al. | 2020 | 2.99 | 3.77 | β | 1 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.75 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.75 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 4.77 | 4.01 | β | 1 | β | β | β | β |
| Kharchenko et al. | 2013 | 4.77 | 4.01 | β | 1 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 3.94 | β | 22 | β | β | β | 0 |
| van den Bergh | 2006 | 2.80 | 3.94 | β | 22 | β | β | β | β |
| Dias et al. | 2002 | 3.60 | 3.79 | β | 10 | 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: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.11 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.11 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0908, e_all=0.1013.