Pismis 27
(MWSC 780)
0.71
UTI
0.75
CN
0.94
Cdens
0.75
CC3
0.71
Clit
0.92
Cdup
Nm (P>50%)
112
Core radius and density
1.5 [pc], 4.7 [pc-2]
- CN 0.75 Rich
- Cdens 0.94 Very dense
- CC3 0.75 High quality
- Clit 0.71 Moderately studied
- Cdup 0.92 Very likely unique
Overview
Pismis 27 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 parameter (see Parameters). It is moderately studied in the literature.
Note: This is very likely a unique object, which shares a very small 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 | 99999â | 92.726 | 20.618 | 0.508 | -0.187 | -2.048 | 32.501 |
| Almeida et al. | 2025 | 92.72 | 20.622 | â | â | â | â |
| Zhang et al. | 2024 | 92.726 | 20.62 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.726 | 20.62 | 0.512 | -0.237 | -2.097 | -7.869 |
| Celli et al. | 2024 | 92.719 | 20.617 | â | â | â | â |
| Cavallo et al. | 2024 | 92.765 | 20.618 | 0.512 | â | â | â |
| Hunt & Reffert | 2023 | 92.726 | 20.62 | 0.512 | -0.237 | -2.097 | -7.869 |
| Almeida et al. | 2023 | 92.717 | 20.62 | â | â | â | â |
| Just et al. | 2023 | 92.721 | 20.616 | â | â | â | â |
| Dias et al. | 2021 | 92.72 | 20.622 | 0.485 | -0.14 | -1.988 | â |
| Cantat-Gaudin et al. | 2020 | 92.719 | 20.617 | 0.504 | -0.14 | -1.994 | â |
| Zhong et al. | 2020 | 92.719 | 20.617 | â | -0.14 | -1.994 | -3.505 |
| Cantat-Gaudin & Anders | 2020 | 92.719 | 20.617 | 0.504 | -0.14 | -1.994 | â |
| Cantat-Gaudin et al. | 2018 | 92.719 | 20.617 | 0.504 | -0.14 | -1.994 | â |
| Dib et al. | 2018 | 92.73 | 20.615 | â | â | â | â |
| Loktin & Popova | 2017 | 92.73 | 20.607 | â | 0.044 | -1.939 | â |
| Sampedro et al. | 2017 | 92.725 | 20.607 | â | 2.9 | -4.45 | â |
| Joshi et al. | 2016 | 92.73 | 20.615 | â | â | â | â |
| Kharchenko et al. | 2016 | 92.721 | 20.616 | â | â | â | â |
| Kharchenko et al. | 2013 | 92.73 | 20.615 | â | 0.98 | -4.03 | â |
| Bukowiecki et al. | 2011 | 92.729 | 20.614 | â | â | â | â |
| Glushkova et al. | 2010 | 92.724 | 20.607 | â | â | â | â |
| Dias et al. | 2002 | 92.725 | 20.607 | â | -5.7 | 24.77 | 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 | 1.74 | 1.91 | 2.015 | 42 | -0.098 | 198 | 0.75 | â |
| Almeida et al. | 2025 | 1.74 | 1.83 | â | 9 | â | 272 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.182(1) | â | â | â |
| Hunt & Reffert | 2024 | 1.83 | 1.68 | 2.01 | 11 | â | 191(1) | â | â |
| Celli et al. | 2024 | â | â | â | 5 | â | 212 | â | â |
| Cavallo et al. | 2024 | 1.68 | 1.87 | â | 35 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 1.83 | 1.68 | 2.02 | 11 | â | â | â | â |
| Almeida et al. | 2023 | 1.76 | 2.16 | â | 9 | -0.098 | 205(1) | 0.75 | â |
| Just et al. | 2023 | â | â | â | 178 | â | 45 | â | â |
| Dias et al. | 2021 | 1.74 | 1.83 | â | 9 | 0.101 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.89 | 1.50 | â | 5 | â | â | â | â |
| Kounkel et al. | 2020 | 1.81 | 2.05 | â | 87 | â | â | â | â |
| Zhong et al. | 2020 | 1.88(1) | â | â | â | -0.528 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.88 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.88 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.66 | â | â | 178 | â | â | â | â |
| Loktin & Popova | 2017 | 2.49 | 1.77 | â | 85 | â | â | â | â |
| Joshi et al. | 2016 | 1.66 | 1.91 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.66 | 1.91 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.66 | 1.91 | â | 178 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 176 | â | â |
| Bukowiecki et al. | 2011 | 1.74(1) | 2.24 | â | 25 | â | â | â | â |
| Glushkova et al. | 2010 | 1.00 | 2.15 | â | 50 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 2.15 | â | 50 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G118, along with HSC_1504, NGC_2175, UBC_1303 and FSR_0902.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.81 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.81 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1042, e_all=0.1613.