Pismis 24
0.63
UTI
0.71
CN
1.0
Cdens
0.75
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
7.8 [N/pc2]
- CN 0.71 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
Pismis 24 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. 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 | 261.397 | -34.363 | 0.56 | -0.947 | -2.53 | 9.47 |
| Jaehnig et al. | 2021 | 261.391 | -34.402 | 0.572 | -0.978 | -2.502 | â |
| Morales et al. | 2013 | 261.179 | -34.206 | â | â | â | â |
| Bukowiecki et al. | 2011 | 261.387 | -34.435 | â | â | â | â |
| van den Bergh | 2006 | 261.35 | -34.433 | â | â | â | â |
| Dias et al. | 2002 | 261.179 | -34.206 | â | 2.29 | -0.91 | 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 | 1.89 | 5.33 | â | 10 | â | 631 | â | â |
| Jaehnig et al. | 2021 | 1.75(1) | â | â | â | â | â | â | â |
| Morales et al. | 2013 | 1.74 | â | â | 2 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 631 | â | â |
| Bukowiecki et al. | 2011 | 1.89(1) | 5.08 | â | 13 | â | â | â | â |
| van den Bergh | 2006 | 2.00 | 5.33 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 2.00 | 5.33 | â | 10 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster, presence of an IR bubble.