Trumpler 37
0.70
UTI
0.7
CN
0.64
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
29.7 [arcmin]
- CN 0.7 Moderately populated
- Cdens 0.64 Moderately dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Trumpler 37 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 324.572 | 57.777 | 1.642 | -6.102 | -5.949 | -3.024 |
| Hu & Soubiran | 2025 | 324.955 | 57.824 | â | â | â | â |
| Hunt & Reffert | 2024 | 324.648 | 57.768 | 1.639 | -6.141 | -5.965 | -3.615 |
| Cavallo et al. | 2024 | 324.955 | 57.824 | 1.641 | â | â | â |
| Hunt & Reffert | 2023 | 324.648 | 57.768 | 1.639 | -6.141 | -5.965 | -3.615 |
| Jaehnig et al. | 2021 | 324.77 | 57.504 | 1.105 | -2.318 | -4.724 | â |
| Loktin & Popova | 2017 | 324.78 | 57.5 | â | -1.016 | -0.968 | â |
| Dias et al. | 2014 | 324.775 | 57.5 | â | -0.19 | -4.29 | â |
| Gozha et al. | 2012 | 324.775 | 57.5 | â | â | â | â |
| van den Bergh | 2006 | 324.536 | 57.447 | â | â | â | â |
| Chen et al. | 2003 | 324.801 | 57.467 | â | -2.95 | -4.57 | 22.3 |
| Dias et al. | 2002 | 324.775 | 57.5 | â | -1.58 | -1.7 | -19.06 |
| Dambis | 1999 | 324.536 | 57.447 | 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 | 0.83 | 1.46 | 2.27 | 11 | 0.105 | 1408 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.110(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 62(1) | â | â |
| Cavallo et al. | 2024 | 0.64 | 1.34 | â | 513 | 0.320 | â | â | â |
| Hunt & Reffert | 2023 | 0.59 | 1.52 | 2.27 | 285 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.90(1) | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.84 | 1.47 | â | 11 | â | â | â | â |
| Gozha et al. | 2012 | 0.83 | â | â | 11 | â | 2754 | â | â |
| van den Bergh | 2006 | 0.83 | 1.46 | â | 11 | â | â | â | â |
| Chen et al. | 2003 | 0.83 | â | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 0.83 | 1.46 | â | 11 | â | â | â | â |
| Dambis | 1999 | 0.81 | 1.43 | â | 10 | â | â | â | â |
(N): Indicates that are N extra values assigned to this parameter in the corresponding reference.


Cavallo et al. (2024)
Gold sample.