ASCC 82
(MWSC 2320)
0.27
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.54
Clit
1.0
Cdup
Nm (P>50%)
20
Core radius and density
9.0 [pc], 0.04 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.54 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 82 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.23 kpc) differs significantly from the median photometric distance (~0.80 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 236.868 | -64.426 | 0.236 | -3.093 | -3.746 | -46.862 |
| Just et al. | 2023 | 236.746 | -64.41 | â | â | â | â |
| Bica et al. | 2019 | 236.841 | -64.412 | â | â | â | â |
| Dib et al. | 2018 | 236.76 | -64.412 | â | â | â | â |
| Sampedro et al. | 2017 | 236.85 | -64.41 | â | -4.51 | -4.3 | â |
| Joshi et al. | 2016 | 236.76 | -64.412 | â | â | â | â |
| Kharchenko et al. | 2016 | 236.746 | -64.41 | â | â | â | â |
| Dias et al. | 2014 | 236.85 | -64.41 | â | -4.52 | -4.31 | â |
| Kharchenko et al. | 2013 | 236.76 | -64.412 | â | -2.34 | -5.16 | â |
| Piskunov et al. | 2008 | 236.84 | -64.412 | â | â | â | â |
| Kharchenko et al. | 2005 | 236.85 | -64.41 | â | -2.96 | -5.23 | â |
| Dias et al. | 2002 | 236.85 | -64.41 | â | -4.52 | -4.31 | 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 | 0.8 | 0.0 | â | 398 | â | 197 | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 22 | â | â |
| Dib et al. | 2018 | 0.80 | â | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 0.80 | 0.00 | â | 398 | â | 372 | â | â |
| Kharchenko et al. | 2016 | 0.80 | 0.00 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.80 | 0.00 | â | 398 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.00 | â | 468 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.00 | â | 468 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.00 | â | 468 | â | â | â | â |
MOCA
