Pismis 19
(VDBH 160; MWSC 2225; OCL 921; vdBergh-Hagen 160; ESO 134 05; FSR 1679)
0.85
UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.71
Clit
1.0
Cdup
Nm (P>50%)
314
Core radius and density
0.8 [pc], 34 [pc-2]
- CN 0.83 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.71 Moderately 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 very massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate 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 | 99999â | 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 |
| Jadhav & Subramaniam | 2021 | 217.666 | -60.889 | 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 |
| Dias et al. | 2018 | â | â | â | -5.18 | -3.7 | â |
| Dib et al. | 2018 | 217.65 | -60.885 | â | â | â | â |
| Sampedro et al. | 2017 | 217.667 | -60.883 | â | -5.71 | -5.59 | 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 |
| Morales et al. | 2013 | 217.664 | -60.883 | â | â | â | â |
| Bukowiecki et al. | 2011 | 217.658 | -60.887 | â | â | â | 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 |
| Lynga | 1987 | 217.665 | -60.968 | â | â | â | â |
| van den Bergh & Hagen | 1975 | 216.725 | -60.667 | â | â | â | 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 | 2.9 | 4.1 | 2.795 | 852 | 0.170 | 5272 | â | 0 |
| Hunt & Reffert | 2024 | 3.03 | 4.94 | 2.80 | 123 | â | 7088(1) | 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 |
| Jadhav & Subramaniam | 2021 | 3.52 | 3.66 | â | 832 | â | 13615 | â | 0(1) |
| Cantat-Gaudin et al. | 2020 | 3.52 | 3.66 | â | 832 | â | â | â | â |
| Kounkel et al. | 2020 | 2.77 | 3.84 | â | 871 | 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 |
| Dib et al. | 2018 | 1.98 | â | â | 1035 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.98 | 4.10 | â | 1035 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.98 | 4.10 | â | 1035 | â | â | â | â |
| Morales et al. | 2013 | 2.40 | â | â | 1122 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 3456 | â | â |
| Bukowiecki et al. | 2011 | 2.41(1) | 3.66 | â | 794 | â | â | â | â |
| van den Bergh | 2006 | 2.40 | 4.57 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 4.67 | â | 794 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.14 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.14 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1083, e_all=0.1004.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg45' along with Hogg 17, NGC 5617 and Trumpler 22.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.