ASCC 119
(MWSC 3614)
0.54
UTI
0.77
CN
0.32
Cdens
0.62
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
6.5 [arcmin]
- 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).
Relatively close
Low extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 334.729 | 46.896 | 0.193 | -3.094 | -2.994 | -50.764 |
| Just et al. | 2023 | 334.658 | 46.881 | – | – | – | – |
| Bica et al. | 2019 | 334.8 | 46.897 | – | – | – | – |
| Kharchenko et al. | 2016 | 334.658 | 46.881 | – | – | – | – |
| Kharchenko et al. | 2013 | 334.665 | 46.885 | – | -4.88 | -5.5 | – |
| Kharchenko et al. | 2012 | 334.665 | 46.885 | – | -4.88 | -5.5 | – |
| Piskunov et al. | 2008 | 334.8 | 46.897 | – | – | – | – |
| Kharchenko et al. | 2005 | 334.8 | 46.9 | – | -6.15 | -6.06 | – |
| Dias et al. | 2002 | 334.8 | 46.9 | – | -1.52 | -2.42 | – |
💡 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 | – | – | – | 618 | – | 104 | – | – |
| Kharchenko et al. | 2016 | 1.20 | 0.31 | – | 618 | – | – | – | – |
| Kharchenko et al. | 2013 | 1.20 | 0.31 | – | 618 | – | – | – | – |
| Kharchenko et al. | 2012 | 1.20 | 0.31 | – | 618 | – | – | – | – |
| Piskunov et al. | 2008 | 1.00 | 0.31 | – | 676 | – | – | – | – |
| Kharchenko et al. | 2005 | 1.00 | 0.31 | – | 676 | – | – | – | – |
| Dias et al. | 2002 | 1.00 | 0.31 | – | 676 | – | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
