Hogg 17
(MWSC 2232)
0.93
UTI
0.65
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
11.6 [N/pc2]
- CN 0.65 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Hogg 17 is a moderately populated, very dense object of very high 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, intermediate-age cluster, but with a large variance across recent sources for the absorption and mass parameters (see Parameters). It is very 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 | 218.458 | -61.326 | 0.411 | -5.234 | -2.422 | -44.142 |
| Liu et al. | 2025 | 218.47 | -61.31 | 0.41 | -5.25 | -2.42 | -43.93 |
| Li et al. | 2025 | 218.459 | -61.326 | 0.407 | -5.201 | -2.433 | â |
| Almeida et al. | 2025 | 218.464 | -61.328 | â | â | â | â |
| Hunt & Reffert | 2024 | 218.468 | -61.313 | 0.414 | -5.247 | -2.423 | -43.925 |
| Cavallo et al. | 2024 | 218.478 | -61.324 | 0.414 | â | â | â |
| Hunt & Reffert | 2023 | 218.468 | -61.313 | 0.414 | -5.247 | -2.423 | -43.925 |
| Just et al. | 2023 | 218.485 | -61.344 | â | â | â | â |
| Jaehnig et al. | 2021 | 218.451 | -61.36 | 0.438 | -5.21 | -2.439 | â |
| Rain et al. | 2021 | 218.459 | -61.326 | 0.407 | -5.201 | -2.433 | â |
| Richer et al. | 2021 | 218.473 | -61.333 | 0.377 | -5.213 | -2.443 | â |
| Dias et al. | 2021 | 218.464 | -61.328 | 0.413 | -5.188 | -2.45 | -43.793 |
| Cantat-Gaudin et al. | 2020 | 218.459 | -61.326 | 0.407 | -5.201 | -2.433 | â |
| Cantat-Gaudin & Anders | 2020 | 218.459 | -61.326 | 0.407 | -5.201 | -2.433 | â |
| Soubiran et al. | 2018 | 218.459 | -61.326 | â | â | â | -43.76 |
| Cantat-Gaudin et al. | 2018 | 218.459 | -61.326 | 0.407 | -5.201 | -2.433 | â |
| Loktin & Popova | 2017 | 218.49 | -61.368 | â | -8.429 | -5.605 | â |
| Kharchenko et al. | 2016 | 218.485 | -61.344 | â | â | â | â |
| Dias et al. | 2014 | 218.492 | -61.367 | â | -6.01 | -5.87 | â |
| Kharchenko et al. | 2013 | 218.497 | -61.347 | â | -2.82 | -4.48 | â |
| Morales et al. | 2013 | 218.492 | -61.367 | â | â | â | â |
| van den Bergh | 2006 | 218.458 | -61.363 | â | â | â | â |
| Dias et al. | 2002 | 218.492 | -61.367 | â | -6.01 | -5.87 | 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 | 2.17 | 1.835 | 0.48 | 107 | 0.209 | 283 | â | 0.0 |
| Liu et al. | 2025 | 4.66 | 0.67 | â | 81 | â | â | â | â |
| Li et al. | 2025 | 2.01 | 2.00 | â | 120 | -0.005 | â | â | â |
| Almeida et al. | 2025 | 2.17 | 1.94 | â | 88 | â | 283 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 447(1) | â | â |
| Cavallo et al. | 2024 | 1.70 | 1.72 | â | 219 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.22 | 1.83 | 0.48 | 70 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 141 | â | 15 | â | â |
| Jaehnig et al. | 2021 | 2.31(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.29 | 1.83 | â | 107 | â | â | â | 0 |
| Richer et al. | 2021 | â | 0.53 | â | â | â | â | â | â |
| Dias et al. | 2021 | 2.17 | 1.94 | â | 88 | 0.209 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.28 | 1.80 | â | 148 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.29 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.29 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.29 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.32 | 1.84 | â | 99 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.15 | 1.94 | â | 141 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.15 | 1.94 | â | 141 | â | â | â | â |
| Morales et al. | 2013 | 1.31 | â | â | 107 | â | â | â | â |
| van den Bergh | 2006 | 1.31 | 1.83 | â | 107 | â | â | â | â |
| Dias et al. | 2002 | 1.31 | 1.84 | â | 107 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 261 along with NGC_5617, and of multiple system 73 along with UBC_1527 and NGC_5617.
Palma et al. (2025)
Classified as optical pair P351, along with CWNU_2431.
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg45' along with NGC 5617, Pismis 19 and Trumpler 22.
Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.