Trumpler 28
(Collinder 337; VDBH 238; MWSC 2641; OCL 1029; vdBergh-Hagen 238; ESO 455 25; FoF 2243)
0.91
UTI
0.79
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
42.2 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Trumpler 28 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Note: This object shares a significant percentage of members with 3 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 | 264.224 | -32.464 | 0.646 | -0.844 | -2.826 | -48.36 |
| Almeida et al. | 2025 | 264.236 | -32.468 | â | â | â | â |
| Hunt & Reffert | 2024 | 264.232 | -32.476 | 0.659 | -0.828 | -2.813 | -35.935 |
| Cavallo et al. | 2024 | 264.22 | -32.459 | 0.665 | â | â | â |
| Hunt & Reffert | 2023 | 264.232 | -32.476 | 0.659 | -0.828 | -2.813 | -35.935 |
| Just et al. | 2023 | 264.246 | -32.481 | â | â | â | â |
| Jaehnig et al. | 2021 | 264.231 | -32.466 | 0.736 | -0.771 | -2.815 | â |
| Rain et al. | 2021 | 264.231 | -32.469 | 0.678 | -0.851 | -2.824 | â |
| Dias et al. | 2021 | 264.236 | -32.468 | 0.669 | -0.833 | -2.79 | -39.396 |
| Cantat-Gaudin et al. | 2020 | 264.231 | -32.469 | 0.678 | -0.851 | -2.824 | â |
| Cantat-Gaudin & Anders | 2020 | 264.231 | -32.469 | 0.678 | -0.851 | -2.824 | â |
| Liu & Pang | 2019 | 264.219 | -32.482 | 0.704 | -0.826 | -2.796 | â |
| Dias et al. | 2019 | 264.229 | -32.469 | 0.678 | -0.851 | -2.824 | -15.81 |
| Soubiran et al. | 2018 | 264.231 | -32.469 | â | â | â | -23.47 |
| Bica et al. | 2019 | 264.209 | -32.473 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 264.231 | -32.469 | 0.678 | -0.851 | -2.824 | â |
| Loktin & Popova | 2017 | 264.255 | -32.484 | â | -0.418 | -1.86 | 7.0 |
| Kharchenko et al. | 2016 | 264.246 | -32.481 | â | â | â | â |
| Dias et al. | 2014 | 264.25 | -32.483 | â | -0.56 | -1.8 | â |
| Kharchenko et al. | 2013 | 264.255 | -32.48 | â | -0.78 | -1.78 | 7.0 |
| Gozha et al. | 2012 | 264.25 | -32.483 | â | â | â | â |
| Piskunov et al. | 2008 | 264.246 | -32.481 | â | â | â | â |
| van den Bergh | 2006 | 264.25 | -32.483 | â | â | â | â |
| Kharchenko et al. | 2005 | 264.25 | -32.48 | â | 0.78 | -2.12 | â |
| Kharchenko et al. | 2003 | 264.21 | -32.47 | â | 1.72 | -2.21 | â |
| Dias et al. | 2002 | 264.25 | -32.483 | â | -0.56 | -1.8 | 7.0 |
| Dambis | 1999 | 264.25 | -32.483 | 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 | 1.355 | 2.26 | 1.29 | 19 | 0.212 | 427 | â | 0.0 |
| Almeida et al. | 2025 | 1.35 | 2.24 | â | 19 | â | 480 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 588(1) | â | â |
| Cavallo et al. | 2024 | 1.30 | 2.71 | â | 14 | -1.010 | â | â | â |
| Hunt & Reffert | 2023 | 1.41 | 2.35 | 1.29 | 55 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 4 | â | 374 | â | â |
| Tarricq et al. | 2022 | 1.35 | â | â | 93 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.36(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 1.42 | 2.26 | â | 19 | â | â | â | 0 |
| Dias et al. | 2021 | 1.35 | 2.24 | â | 19 | 0.174 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.40 | 1.79 | â | 78 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.42 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 295 | 0.250 | â | â | â |
| Dias et al. | 2019 | 1.38 | 1.77 | â | 32 | 0.112 | â | â | â |
| Soubiran et al. | 2018 | 1.42 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.42 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.36 | 2.32 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.47 | 2.97 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.47 | 2.97 | â | 4 | 0.326 | â | â | â |
| Gozha et al. | 2012 | 1.34 | â | â | 19 | â | 214 | â | â |
| Piskunov et al. | 2008 | 1.34 | 2.26 | â | 8 | â | â | â | â |
| van den Bergh | 2006 | 1.34 | 2.26 | â | 19 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.34 | 2.26 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.34 | 2.26 | â | â | â | â | â | â |
| Dias et al. | 2002 | 1.34 | 2.27 | â | 19 | 0.326 | â | â | â |
| Dambis | 1999 | 1.23 | 2.36 | â | 22 | 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: intermediate fit. Isochrone match: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.