Pismis 2
(VDBH 25; MWSC 1465; OCL 733; vdBergh-Hagen 25; ESO 312 02; FSR 1392)
0.89
UTI
1.0
CN
1.0
Cdens
0.75
CC3
0.84
Clit
1.0
Cdup
Nm (P>50%)
1029
Core radius and density
1.3 [pc], 49 [pc-2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Pismis 2 is a very rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as an extremely massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the absorption and mass parameters (see Parameters). It is well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a very small percentage of members with 2 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 | 99999β | 124.478 | -41.672 | 0.246 | -4.708 | 5.357 | 60.066 |
| Hu & Soubiran | 2025 | 124.483 | -41.673 | β | β | β | β |
| Hunt & Reffert | 2024 | 124.475 | -41.672 | 0.243 | -4.705 | 5.373 | 59.618 |
| Cavallo et al. | 2024 | 124.483 | -41.673 | 0.243 | β | β | β |
| Hunt & Reffert | 2023 | 124.475 | -41.672 | 0.243 | -4.705 | 5.373 | 59.618 |
| Just et al. | 2023 | 124.486 | -41.667 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 124.477 | -41.674 | β | β | β | β |
| Jaehnig et al. | 2021 | 124.478 | -41.675 | 0.223 | -4.783 | 5.351 | β |
| Rain et al. | 2021 | 124.477 | -41.674 | 0.221 | -4.756 | 5.325 | β |
| Cantat-Gaudin et al. | 2020 | 124.477 | -41.674 | 0.221 | -4.756 | 5.325 | β |
| SΓ‘nchez et al. | 2020 | 124.475 | -41.667 | β | -4.837 | 5.518 | β |
| Cantat-Gaudin & Anders | 2020 | 124.477 | -41.674 | 0.221 | -4.756 | 5.325 | β |
| Soubiran et al. | 2018 | 124.477 | -41.674 | β | β | β | 58.99 |
| Bica et al. | 2019 | 124.483 | -41.661 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 124.477 | -41.674 | 0.221 | -4.756 | 5.325 | β |
| Sampedro et al. | 2017 | 124.475 | -41.667 | β | -5.88 | 1.82 | β |
| Kharchenko et al. | 2016 | 124.486 | -41.667 | β | β | β | β |
| Netopil et al. | 2016 | 124.491 | -41.67 | β | β | β | β |
| Dias et al. | 2014 | 124.475 | -41.667 | β | -5.72 | 0.89 | β |
| Kharchenko et al. | 2013 | 124.491 | -41.67 | β | -4.63 | 6.78 | 49.0 |
| Gozha et al. | 2012 | 124.475 | -41.667 | β | β | β | β |
| Bukowiecki et al. | 2011 | 124.483 | -41.669 | β | β | β | β |
| Kharchenko et al. | 2007 | 124.47 | -41.67 | β | 0.03 | β | β |
| Ahumada & Lapasset | 2007 | 124.475 | -41.667 | β | β | β | β |
| van den Bergh | 2006 | 124.479 | -41.672 | β | β | β | β |
| Dias et al. | 2002 | 124.475 | -41.667 | β | -5.72 | 0.89 | -49.0 |
| Lynga | 1987 | 124.512 | -41.622 | β | β | β | β |
| van den Bergh & Hagen | 1975 | 124.075 | -41.45 | 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 | 3.805 | 3.71 | 2.25 | 1148 | -0.070 | 11091 | β | 5 |
| Hu & Soubiran | 2025 | β | β | β | β | -0.180(5) | β | β | β |
| Hunt & Reffert | 2024 | 3.49 | 4.66 | 2.25 | 561 | β | 11091(1) | β | β |
| Cavallo et al. | 2024 | 3.34 | 4.41 | β | 1023 | -0.360 | β | β | β |
| Hunt & Reffert | 2023 | 3.49 | 4.66 | 2.25 | 561 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 1135 | β | 1380 | β | β |
| Jadhav & Subramaniam | 2021 | 4.07 | 3.32 | β | 1862 | β | 16152 | β | 5(1) |
| Jaehnig et al. | 2021 | 4.59(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 4.00 | 0.16 | β | 1148 | β | β | β | 0 |
| Cantat-Gaudin et al. | 2020 | 4.07 | 3.32 | β | 1862 | β | β | β | β |
| Kounkel et al. | 2020 | 3.62 | 3.71 | β | 1047 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.00 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.00 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.00 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.75 | 4.07 | β | 1135 | β | β | β | β |
| Netopil et al. | 2016 | 9.16 | β | β | 1470 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.75 | 4.07 | β | 1135 | -0.070 | β | β | β |
| Gozha et al. | 2012 | 3.31 | β | β | 1148 | -0.070 | β | β | β |
| Bukowiecki et al. | 2011 | 3.99(1) | 3.19 | β | 1585 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 4.10 | β | 1148 | β | β | β | 46 |
| van den Bergh | 2006 | 3.31 | 0.16 | β | 1148 | β | β | β | β |
| Dias et al. | 2002 | 3.31 | 0.16 | β | 1148 | -0.070 | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.80 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.80 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0384, e_all=0.044.
Ahumada & Lapasset (2007)
Only straggler candidates inside a radius of 3' around the centre of coordinates have been considered.