ASCC 69
(MWSC 1996)
0.40
UTI
0.0
CN
0.26
Cdens
0.38
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
1.3 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.26 Loose
- CC3 0.38 Low quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 69 is a sparse, 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 near-solar metallicity, 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 | 181.663 | -69.866 | 1.348 | -6.497 | -1.932 | 9.124 |
| Cavallo et al. | 2024 | 181.549 | -70.103 | 1.345 | â | â | â |
| Hunt & Reffert | 2023 | 181.594 | -69.857 | 1.342 | -6.454 | -1.89 | 4.676 |
| Just et al. | 2023 | 181.566 | -69.777 | â | â | â | â |
| Bica et al. | 2019 | 181.658 | -69.773 | â | â | â | â |
| Kharchenko et al. | 2016 | 181.566 | -69.777 | â | â | â | â |
| Dias et al. | 2014 | 181.65 | -69.77 | â | -5.52 | 2.56 | â |
| Kharchenko et al. | 2013 | 181.575 | -69.78 | â | -6.9 | 0.5 | 2.0 |
| Gozha et al. | 2012 | 181.65 | -69.77 | â | â | â | â |
| Piskunov et al. | 2008 | 181.635 | -69.762 | â | â | â | â |
| Kharchenko et al. | 2007 | 181.65 | -69.77 | â | 0.4 | â | 2.0 |
| Kharchenko et al. | 2005 | 181.65 | -69.77 | â | -7.52 | -0.64 | 2.0 |
| Dias et al. | 2002 | 181.65 | -69.77 | â | -7.52 | -0.64 | -0.99 |
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 | 0.885 | 0.53 | 0.29 | 81 | 0.470 | 950 | â | â |
| Cavallo et al. | 2024 | 0.74 | 0.64 | â | 115 | 0.470 | â | â | â |
| Hunt & Reffert | 2023 | 0.71 | 0.61 | 0.29 | 73 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 81 | â | 79 | â | â |
| Kharchenko et al. | 2016 | 0.77 | 0.53 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.77 | 0.53 | â | 81 | â | â | â | â |
| Gozha et al. | 2012 | 1.00 | â | â | 81 | â | 1820 | â | â |
| Piskunov et al. | 2008 | 1.00 | 0.53 | â | 81 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 0.53 | â | 81 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.53 | â | 81 | â | â | â | â |
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.