Pismis 17
(OCL 833; MWSC 1882)
0.76
UTI
0.56
CN
1.0
Cdens
0.5
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
10.4 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Pismis 17 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 165.397 | -59.89 | 0.369 | -6.908 | 2.347 | -8.578 |
| Hunt & Reffert | 2024 | 165.354 | -59.87 | 0.363 | -6.908 | 2.37 | -15.426 |
| Celli et al. | 2024 | 165.377 | -59.873 | â | â | â | â |
| Cavallo et al. | 2024 | 165.383 | -59.883 | 0.361 | â | â | â |
| Hunt & Reffert | 2023 | 165.354 | -59.87 | 0.363 | -6.908 | 2.37 | -15.426 |
| Cantat-Gaudin et al. | 2020 | 165.377 | -59.873 | 0.366 | -6.938 | 2.333 | â |
| Cantat-Gaudin & Anders | 2020 | 165.377 | -59.873 | 0.366 | -6.938 | 2.333 | â |
| Bica et al. | 2019 | 165.315 | -59.847 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 165.377 | -59.873 | 0.366 | -6.938 | 2.333 | â |
| Loktin & Popova | 2017 | 165.27 | -59.817 | â | -3.89 | 0.59 | -17.8 |
| Dias et al. | 2014 | 165.275 | -59.817 | â | -3.89 | 0.59 | â |
| Gozha et al. | 2012 | 165.275 | -59.817 | â | â | â | â |
| Piskunov et al. | 2008 | 165.254 | -59.866 | â | â | â | â |
| Kharchenko et al. | 2007 | 165.27 | -59.82 | â | 0.17 | â | 61.7 |
| van den Bergh | 2006 | 165.267 | -59.818 | â | â | â | â |
| Kharchenko et al. | 2005 | 165.27 | -59.87 | â | -6.27 | 3.12 | 61.7 |
| Dias et al. | 2002 | 165.275 | -59.817 | â | -3.89 | 0.59 | 65.1 |
| Dambis | 1999 | 165.267 | -59.818 | 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 | 3.5 | 1.46 | 2.26 | 16 | -0.037 | 516 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 516(1) | â | â |
| Celli et al. | 2024 | â | â | â | 25 | â | 143 | â | â |
| Cavallo et al. | 2024 | 1.86 | 0.77 | â | 72 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 2.51 | 1.31 | 2.26 | 37 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.53 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.53 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.50 | 1.46 | â | 11 | â | â | â | â |
| Gozha et al. | 2012 | 3.50 | â | â | 11 | â | 9772 | â | â |
| Piskunov et al. | 2008 | 3.50 | 1.46 | â | 21 | â | â | â | â |
| van den Bergh | 2006 | 3.50 | 1.46 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2005 | 3.50 | 1.46 | â | 21 | â | â | â | â |
| Dias et al. | 2002 | 3.50 | 1.46 | â | 11 | -0.145 | â | â | â |
| Dambis | 1999 | 4.57 | 1.38 | â | 3 | 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)
Bronze sample.