ASCC 119
(MWSC 3614)
0.54
UTI
0.77
CN
0.32
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
1.6 [N/pc2]
- CN 0.77 Rich
- Cdens 0.32 Loose
- CC3 0.62 Intermediate quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 119 is a rich, loose object of intermediate C3 quality. Its parallax locates it at a large* 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 (~5.19 kpc) differs significantly from the median photometric distance (~1.10 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 334.729 | 46.896 | 0.193 | -3.094 | -2.994 | -50.764 |
| Just et al. | 2023 | 334.658 | 46.881 | â | â | â | â |
| Bica et al. | 2019 | 334.8 | 46.897 | â | â | â | â |
| Kharchenko et al. | 2016 | 334.658 | 46.881 | â | â | â | â |
| Dias et al. | 2014 | 334.8 | 46.9 | â | -1.52 | -2.42 | â |
| Kharchenko et al. | 2013 | 334.665 | 46.885 | â | -4.88 | -5.5 | â |
| Kharchenko et al. | 2012 | 334.665 | 46.885 | â | -4.88 | -5.5 | â |
| Piskunov et al. | 2008 | 334.8 | 46.897 | â | â | â | â |
| Kharchenko et al. | 2005 | 334.8 | 46.9 | â | -6.15 | -6.06 | â |
| Dias et al. | 2002 | 334.8 | 46.9 | â | -1.52 | -2.42 | 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 | 1.1 | 0.31 | â | 618 | â | 104 | â | â |
| Just et al. | 2023 | â | â | â | 618 | â | 104 | â | â |
| Kharchenko et al. | 2016 | 1.20 | 0.31 | â | 618 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.20 | 0.31 | â | 618 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.20 | 0.31 | â | 618 | â | â | â | â |
| Piskunov et al. | 2008 | 1.00 | 0.31 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 0.31 | â | 676 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.31 | â | 676 | â | â | â | â |
MOCA
