Pismis 19
(VDBH 160; MWSC 2225; OCL 921; vdBergh-Hagen 160; ESO 134 05; FSR 1679)
0.88
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Pismis 19 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.
Distant
High extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 217.669 | -60.887 | 0.253 | -5.475 | -3.378 | -30.24 |
| Hunt & Reffert | 2024 | 217.668 | -60.891 | 0.287 | -5.484 | -3.394 | -25.78 |
| Cavallo et al. | 2024 | 217.666 | -60.886 | 0.285 | â | â | â |
| Hunt & Reffert | 2023 | 217.668 | -60.891 | 0.287 | -5.484 | -3.394 | -25.78 |
| Just et al. | 2023 | 217.637 | -60.883 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 217.666 | -60.889 | 0.255 | -5.46 | -3.247 | â |
| Cantat-Gaudin & Anders | 2020 | 217.666 | -60.889 | 0.255 | -5.46 | -3.247 | â |
| Soubiran et al. | 2018 | 217.666 | -60.889 | â | â | â | -29.55 |
| Bica et al. | 2019 | 217.669 | -60.892 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 217.666 | -60.889 | 0.255 | -5.46 | -3.247 | â |
| Kharchenko et al. | 2016 | 217.637 | -60.883 | â | â | â | â |
| Dias et al. | 2014 | 217.667 | -60.883 | â | -2.56 | -6.23 | â |
| Kharchenko et al. | 2013 | 217.65 | -60.885 | â | -1.08 | -1.82 | â |
| van den Bergh | 2006 | 217.675 | -60.983 | â | â | â | â |
| Dias et al. | 2002 | 217.667 | -60.883 | â | -3.07 | -6.01 | 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 | 7088* | â | â |
| Cavallo et al. | 2024 | 3.42 | 4.95 | â | 107 | 0.170 | â | â | â |
| Hunt & Reffert | 2023 | 3.03 | 4.94 | 2.79 | 123 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1035 | â | 32 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.52 | 3.66 | â | 832 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.52 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.52 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.52 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.98 | 4.03 | â | 1035 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.98 | 4.03 | â | 1035 | â | â | â | â |
| van den Bergh | 2006 | 2.40 | 4.50 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 4.59 | â | 794 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.