ASCC 24
(Alessi 47; MWSC 875)
0.39
UTI
0.0
CN
0.55
Cdens
0.75
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
0.8 [pc], 2.7 [pc-2]
- CN 0.0 Sparse
- Cdens 0.55 Moderately dense
- CC3 0.75 High quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
ASCC 24 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a very close* distance, near the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and age parameters (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.21 kpc) differs significantly from the median photometric distance (~0.40 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 97.351 | -7.035 | 4.774 | -7.378 | -2.857 | 18.737 |
| Cavallo et al. | 2024 | 98.287 | -6.882 | 4.727 | â | â | â |
| Hunt & Reffert | 2023 | 97.261 | -7.035 | 4.728 | -7.354 | -2.881 | 35.998 |
| Bica et al. | 2019 | 97.18 | -7.021 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -0.75 | -0.41 | â |
| Sampedro et al. | 2017 | 97.183 | -7.02 | â | 0.77 | -3.56 | â |
| Joshi et al. | 2016 | 97.185 | -6.98 | â | â | â | â |
| Dias et al. | 2014 | 97.183 | -7.02 | â | 0.4 | -3.46 | â |
| Gozha et al. | 2012 | 97.183 | -7.02 | â | â | â | â |
| Piskunov et al. | 2008 | 97.18 | -7.021 | â | â | â | â |
| Kharchenko et al. | 2007 | 97.18 | -7.02 | â | 0.35 | â | 16.35 |
| Kharchenko et al. | 2005 | 97.18 | -7.02 | â | -5.55 | -4.05 | 16.35 |
| Dias et al. | 2002 | 97.183 | -7.02 | â | -5.55 | -4.05 | 15.66 |
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 | 0.4 | 0.44 | 0.48 | 9 | -0.490 | 40 | â | â |
| Cavallo et al. | 2024 | 0.19 | 0.00 | â | 1 | -0.490 | â | â | â |
| Hunt & Reffert | 2023 | 0.22 | 0.39 | 0.48 | 32 | â | â | â | â |
| Joshi et al. | 2016 | 0.38 | 0.46 | â | 20 | â | 40 | â | â |
| Gozha et al. | 2012 | 0.40 | â | â | 9 | â | 40 | â | â |
| Piskunov et al. | 2008 | 0.40 | 0.44 | â | 9 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.40 | 0.44 | â | 9 | â | â | â | â |
| Dias et al. | 2002 | 0.40 | 0.44 | â | 9 | â | â | â | â |
MOCA


Palma et al. (2025)
Classified as optical pair P266, along with HSC_1709.
Cavallo et al. (2024)
Wood sample.
Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.98 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.98 (50th percentile).
Bica et al. (2019)
List of clusters and alike reported by B. Alessi.