ASCC 84
(MWSC 2333)
0.37
UTI
0.0
CN
0.24
Cdens
0.38
CC3
0.62
Clit
1.0
Cdup
Stellar density (N50/rad)
1.2 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.24 Very loose
- CC3 0.38 Low quality
- Clit 0.62 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 84 is a sparse, very loose object of low C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 238.777 | -60.67 | 1.157 | -1.399 | -4.244 | -1.976 |
| Hunt & Reffert | 2023 | 238.683 | -60.713 | 1.152 | -1.36 | -4.201 | -1.962 |
| Just et al. | 2023 | 238.719 | -60.743 | â | â | â | â |
| Bica et al. | 2019 | 238.71 | -60.739 | â | â | â | â |
| Kharchenko et al. | 2016 | 238.719 | -60.743 | â | â | â | â |
| Dias et al. | 2014 | 238.725 | -60.74 | â | -5.49 | -3.44 | â |
| Kharchenko et al. | 2013 | 238.732 | -60.745 | â | -1.92 | -5.54 | -5.0 |
| Gozha et al. | 2012 | 238.725 | -60.74 | â | â | â | â |
| Piskunov et al. | 2008 | 238.71 | -60.739 | â | â | â | â |
| Kharchenko et al. | 2007 | 238.72 | -60.74 | â | 0.25 | â | -5.0 |
| Kharchenko et al. | 2005 | 238.72 | -60.74 | â | -1.74 | -4.87 | -5.0 |
| Dias et al. | 2002 | 238.725 | -60.74 | â | -5.49 | -3.44 | -5.0 |
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 | 0.9 | 0.62 | 0.47 | 48 | â | 108 | â | â |
| Hunt & Reffert | 2023 | 0.85 | 0.78 | 0.47 | 29 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 71 | â | 20 | â | â |
| Kharchenko et al. | 2016 | 0.88 | 0.84 | â | 71 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.88 | 0.84 | â | 71 | â | â | â | â |
| Gozha et al. | 2012 | 0.90 | â | â | 48 | â | 195 | â | â |
| Piskunov et al. | 2008 | 0.90 | 0.46 | â | 48 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.90 | 0.46 | â | 48 | â | â | â | â |
| Dias et al. | 2002 | 0.90 | 0.46 | â | 48 | â | â | â | â |
MOCA


Hunt & Reffert (2024)
Classified as a moving group.