Trumpler 15
(FoF 232)
0.95
UTI
1.0
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
85.9 [N/pc2]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 15 is a very rich, very dense object of 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, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is very well-studied in the literature.
Note: This object shares a very small percentage of members with a later reported entry. 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 | 161.175 | -59.374 | 0.391 | -6.206 | 2.085 | 9.881 |
| Almeida et al. | 2025 | 161.179 | -59.372 | â | â | â | â |
| Hunt & Reffert | 2024 | 161.174 | -59.369 | 0.387 | -6.093 | 2.068 | 23.263 |
| Celli et al. | 2024 | 161.177 | -59.369 | â | â | â | â |
| Cavallo et al. | 2024 | 161.18 | -59.375 | 0.388 | â | â | â |
| Hunt & Reffert | 2023 | 161.174 | -59.369 | 0.387 | -6.093 | 2.068 | 23.263 |
| Almeida et al. | 2023 | 161.186 | -59.372 | â | â | â | â |
| Jaehnig et al. | 2021 | 161.093 | -59.533 | 0.419 | -6.413 | 2.039 | â |
| Rain et al. | 2021 | 161.177 | -59.369 | 0.398 | -6.209 | 2.016 | â |
| Dias et al. | 2021 | 161.179 | -59.372 | 0.396 | -6.188 | 2.017 | â |
| Cantat-Gaudin et al. | 2020 | 161.177 | -59.369 | 0.398 | -6.209 | 2.016 | â |
| Cantat-Gaudin & Anders | 2020 | 161.177 | -59.369 | 0.398 | -6.209 | 2.016 | â |
| Liu & Pang | 2019 | 161.176 | -59.372 | 0.398 | -6.192 | 2.064 | â |
| Dias et al. | 2019 | 161.179 | -59.369 | 0.398 | -6.209 | 2.016 | 16.59 |
| Cantat-Gaudin et al. | 2018 | 161.177 | -59.369 | 0.398 | -6.209 | 2.016 | â |
| Loktin & Popova | 2017 | 161.175 | -59.367 | â | -7.71 | 3.26 | -13.2 |
| Dias et al. | 2014 | 161.179 | -59.367 | â | -4.13 | 0.19 | â |
| Gozha et al. | 2012 | 161.179 | -59.367 | â | â | â | â |
| Piskunov et al. | 2008 | 161.178 | -59.368 | â | â | â | â |
| Kharchenko et al. | 2007 | 161.17 | -59.37 | â | 0.08 | â | -9.0 |
| van den Bergh | 2006 | 161.175 | -59.367 | â | â | â | â |
| Kharchenko et al. | 2005 | 161.17 | -59.37 | â | -2.08 | 3.53 | â |
| Kharchenko et al. | 2003 | 161.16 | -59.35 | â | -2.44 | 2.91 | â |
| Dias et al. | 2002 | 161.179 | -59.367 | â | -7.71 | 3.26 | -15.06 |
| Dambis | 1999 | 161.179 | -59.367 | 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 | 2.29 | 1.48 | 1.96 | 8 | 0.013 | 925 | 0.67 | 0.0 |
| Almeida et al. | 2025 | 2.29 | 1.61 | â | 7 | â | 1027 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 647(1) | â | â |
| Celli et al. | 2024 | â | â | â | 9 | â | 925 | â | â |
| Cavallo et al. | 2024 | 2.08 | 1.58 | â | 5 | -0.570 | â | â | â |
| Hunt & Reffert | 2023 | 2.40 | 1.69 | 1.96 | 8 | â | â | â | â |
| Almeida et al. | 2023 | 2.30 | 1.64 | â | 8 | 0.013 | 1052(1) | 0.67 | â |
| Jaehnig et al. | 2021 | 2.38(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.34 | 1.33 | â | 8 | â | â | â | 0 |
| Dias et al. | 2021 | 2.29 | 1.61 | â | 7 | -0.124 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.59 | 1.50 | â | 9 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.34 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 8 | 0.500 | â | â | â |
| Dias et al. | 2019 | 3.69 | 1.46 | â | 5 | 1.016 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.34 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.12 | 1.97 | â | 8 | â | â | â | â |
| Gozha et al. | 2012 | 1.85 | â | â | 8 | â | 224 | â | â |
| Piskunov et al. | 2008 | 2.12 | 1.40 | â | 12 | â | â | â | â |
| van den Bergh | 2006 | 1.85 | 1.33 | â | 9 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.12 | 1.40 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.85 | 1.33 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.85 | 1.35 | â | 8 | â | â | â | â |
| Dambis | 1999 | 2.19 | 1.48 | â | 3 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.