Trumpler 24
0.33
UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
58.8 [arcmin]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.38 Low quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Trumpler 24 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very 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 parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~0.42 kpc) differs significantly from the median photometric distance (~1.14 kpc).
Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 254.2 | -40.609 | 2.377 | -3.044 | -7.279 | -14.062 |
| Cavallo et al. | 2024 | 254.284 | -39.929 | 2.39 | â | â | â |
| Hunt & Reffert | 2023 | 254.182 | -40.473 | 2.386 | -3.104 | -7.202 | -14.22 |
| Jaehnig et al. | 2021 | 253.986 | -40.474 | 0.835 | 0.372 | -1.8 | â |
| Loktin & Popova | 2017 | 254.25 | -40.668 | â | -2.641 | -5.822 | -3.45 |
| Dias et al. | 2014 | 254.25 | -40.667 | â | -2.61 | -3.5 | â |
| Gozha et al. | 2012 | 254.25 | -40.667 | â | â | â | â |
| Kharchenko et al. | 2007 | 254.25 | -40.67 | â | 0.5 | â | â |
| van den Bergh | 2006 | 254.25 | -40.667 | â | â | â | â |
| Chen et al. | 2003 | 253.791 | -40.773 | â | 0.3 | -0.17 | -4.0 |
| Dambis | 1999 | 254.25 | -40.667 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.42 | 1.16 | â | 28 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 0.40 | 0.60 | 0.94 | 216 | â | â | â | â |
| Jaehnig et al. | 2021 | 1.20* | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.14 | 1.32 | â | 14 | â | â | â | â |
| Gozha et al. | 2012 | 1.14 | â | â | 8 | â | â | â | â |
| van den Bergh | 2006 | 1.14 | 1.30 | â | 8 | â | â | â | â |
| Chen et al. | 2003 | 1.14 | â | â | 0 | â | â | â | â |
| Dambis | 1999 | 1.41 | 1.26 | â | 8 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.