Trumpler 34
(Collinder 387; MWSC 2970; OCL 69)
0.84
UTI
0.6
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
10.1 [N/pc2]
- CN 0.6 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Trumpler 34 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below 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 age parameter (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 | 99999β | 279.944 | -8.436 | 0.322 | -1.027 | -3.528 | 8.658 |
| Hunt & Reffert | 2024 | 279.957 | -8.43 | 0.329 | -1.053 | -3.543 | 41.794 |
| Cavallo et al. | 2024 | 279.945 | -8.442 | 0.329 | β | β | β |
| He et al. | 2023 | 279.859 | -8.426 | 0.273 | -0.829 | -2.999 | 45.17 |
| Hunt & Reffert | 2023 | 279.957 | -8.43 | 0.329 | -1.053 | -3.543 | 41.794 |
| Just et al. | 2023 | 279.942 | -8.417 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 279.935 | -8.439 | 0.305 | -0.933 | -3.448 | β |
| SΓ‘nchez et al. | 2020 | 279.95 | -8.417 | β | -1.211 | -3.473 | β |
| Cantat-Gaudin & Anders | 2020 | 279.935 | -8.439 | 0.305 | -0.933 | -3.448 | β |
| Soubiran et al. | 2018 | 279.935 | -8.439 | β | β | β | -12.38 |
| Bica et al. | 2019 | 279.951 | -8.428 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 279.935 | -8.439 | 0.305 | -0.933 | -3.448 | β |
| Kharchenko et al. | 2016 | 279.942 | -8.417 | β | β | β | β |
| Dias et al. | 2014 | 279.95 | -8.417 | β | -0.3 | -3.99 | β |
| Kharchenko et al. | 2013 | 279.949 | -8.415 | β | -4.14 | -7.01 | β |
| Dias et al. | 2002 | 279.95 | -8.417 | β | -0.3 | -3.99 | β |
π‘ 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 | 99999β | 2.78 | 2.665 | 0.52 | 385 | -0.220 | 394 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 646(1) | β | β |
| Cavallo et al. | 2024 | 1.87 | 2.82 | β | 214 | -0.220 | β | β | β |
| He et al. | 2023 | 3.02 | 4.55 | β | 126 | β | β | β | β |
| Hunt & Reffert | 2023 | 2.78 | 2.81 | 0.52 | 65 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 385 | β | 143 | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.00 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.00 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.00 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 1.34 | 2.52 | β | 385 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.34 | 2.52 | β | 385 | β | β | β | β |
| Dias et al. | 2002 | 1.34 | 2.52 | β | 385 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.