Pismis 22
(MWSC 2371)
0.85
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
1.1 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Pismis 22 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~6.12 kpc) differs significantly from the median photometric distance (~3.70 kpc).
Distant
Very high extinction
Massive
Metal-rich
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 243.542 | -51.869 | 0.164 | -3.791 | -4.288 | 42.57 |
| Hunt & Reffert | 2024 | 243.543 | -51.873 | 0.183 | -3.797 | -4.259 | 26.919 |
| Cavallo et al. | 2024 | 243.554 | -51.867 | 0.184 | â | â | â |
| Hunt & Reffert | 2023 | 243.543 | -51.873 | 0.183 | -3.797 | -4.259 | 26.919 |
| Just et al. | 2023 | 243.544 | -51.864 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 243.552 | -51.869 | 0.102 | -3.882 | -4.263 | â |
| Cantat-Gaudin & Anders | 2020 | 243.552 | -51.869 | 0.102 | -3.882 | -4.263 | â |
| Soubiran et al. | 2018 | 243.552 | -51.869 | â | â | â | -52.58 |
| Cantat-Gaudin et al. | 2018 | 243.552 | -51.869 | 0.102 | -3.882 | -4.263 | â |
| Kharchenko et al. | 2016 | 243.544 | -51.864 | â | â | â | â |
| Dias et al. | 2014 | 243.538 | -51.867 | â | -2.99 | -3.95 | â |
| Kharchenko et al. | 2013 | 243.555 | -51.865 | â | -10.73 | -3.63 | â |
| van den Bergh | 2006 | 243.537 | -51.867 | â | â | â | â |
| Dias et al. | 2002 | 243.537 | -51.867 | â | -2.97 | -3.31 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 3290* | â | â |
| Cavallo et al. | 2024 | 3.70 | 5.43 | â | 1 | 0.900 | â | â | â |
| Hunt & Reffert | 2023 | 4.86 | 6.45 | 2.65 | 50 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 158 | â | 96 | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.65 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.65 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.02 | 5.97 | â | 158 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.02 | 5.97 | â | 158 | â | â | â | â |
| van den Bergh | 2006 | 1.00 | 6.20 | â | 40 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 6.20 | â | 40 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Wood sample.