ASCC 64
(MWSC 1884)
0.32
UTI
0.0
CN
0.04
Cdens
0.38
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
7.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.04 Very loose
- CC3 0.38 Low quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 64 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.31 kpc) differs significantly from the median photometric distance (~1.50 kpc).
Relatively close
Low extinction
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 165.777 | -60.911 | 0.232 | -6.126 | 2.015 | 12.074 |
| Just et al. | 2023 | 165.758 | -60.911 | â | â | â | â |
| Bica et al. | 2019 | 165.761 | -60.921 | â | â | â | â |
| Kharchenko et al. | 2016 | 165.758 | -60.911 | â | â | â | â |
| Dias et al. | 2014 | 165.767 | -60.92 | â | -2.94 | -3.58 | â |
| Kharchenko et al. | 2013 | 165.765 | -60.915 | â | -5.6 | 1.77 | 1.4 |
| Gozha et al. | 2012 | 165.767 | -60.92 | â | â | â | â |
| Piskunov et al. | 2008 | 165.761 | -60.921 | â | â | â | â |
| Kharchenko et al. | 2007 | 165.76 | -60.92 | â | 0.18 | â | -8.33 |
| Kharchenko et al. | 2005 | 165.76 | -60.92 | â | -5.88 | 1.44 | -8.33 |
| Dias et al. | 2002 | 165.767 | -60.92 | â | -2.94 | -3.58 | 1.15 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 126 | â | 449 | â | â |
| Kharchenko et al. | 2016 | 1.70 | 0.46 | â | 126 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.70 | 0.46 | â | 126 | â | â | â | â |
| Gozha et al. | 2012 | 1.50 | â | â | 83 | â | 617 | â | â |
| Piskunov et al. | 2008 | 1.50 | 0.46 | â | 83 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.50 | 0.46 | â | 83 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 0.46 | â | 83 | â | â | â | â |
