ASCC 28
(MWSC 1011)
0.41
UTI
0.0
CN
0.12
Cdens
0.38
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
0.6 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.12 Very loose
- CC3 0.38 Low quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 28 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low 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 | 99999â | 103.478 | -0.195 | 0.922 | -2.581 | -2.409 | 40.123 |
| Zhang et al. | 2024 | 103.453 | -0.129 | â | â | â | â |
| Hunt & Reffert | 2024 | 103.453 | -0.129 | 0.919 | -2.569 | -2.428 | 48.981 |
| Cavallo et al. | 2024 | 103.46 | -0.23 | 0.918 | â | â | â |
| Hunt & Reffert | 2023 | 103.453 | -0.129 | 0.919 | -2.569 | -2.428 | 48.981 |
| Just et al. | 2023 | 103.568 | -0.148 | â | â | â | â |
| Bica et al. | 2019 | 103.518 | -0.166 | â | â | â | â |
| Kharchenko et al. | 2016 | 103.568 | -0.148 | â | â | â | â |
| Dias et al. | 2014 | 103.517 | -0.17 | â | 0.62 | -2.82 | â |
| Kharchenko et al. | 2013 | 103.575 | -0.15 | â | -2.39 | -0.3 | 22.7 |
| Gozha et al. | 2012 | 103.517 | -0.17 | â | â | â | â |
| Piskunov et al. | 2008 | 103.509 | -0.171 | â | â | â | â |
| Kharchenko et al. | 2007 | 103.51 | -0.17 | â | 0.3 | â | 22.7 |
| Kharchenko et al. | 2005 | 103.51 | -0.17 | â | -1.68 | -1.1 | 22.7 |
| Dias et al. | 2002 | 103.517 | -0.17 | â | -1.68 | -1.1 | 22.7 |
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 | 0.875 | 0.19 | 0.45 | 219 | -0.144 | 92 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.149(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 69(1) | â | â |
| Cavallo et al. | 2024 | 1.06 | 0.56 | â | 68 | -0.140 | â | â | â |
| Hunt & Reffert | 2023 | 1.03 | 0.30 | 0.45 | 95 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 309 | â | 92 | â | â |
| Kharchenko et al. | 2016 | 0.95 | 0.19 | â | 309 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.95 | 0.19 | â | 309 | â | â | â | â |
| Gozha et al. | 2012 | 0.80 | â | â | 219 | â | 224 | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.16 | â | 219 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.16 | â | 219 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.16 | â | 219 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.