ASCC 120
(MWSC 3631)
0.27
UTI
0.0
CN
0.03
Cdens
0.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
7.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.0 Very low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 120 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very massive, very young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.21 kpc) differs significantly from the median photometric distance (~2.50 kpc).
Relatively close
Moderate extinction
Very massive
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 337.631 | 57.226 | 0.238 | -0.756 | -1.966 | â |
| Just et al. | 2023 | 337.561 | 57.191 | â | â | â | â |
| Bica et al. | 2019 | 344.055 | 50.158 | â | â | â | â |
| Kharchenko et al. | 2016 | 337.561 | 57.191 | â | â | â | â |
| Dias et al. | 2014 | 337.65 | 57.21 | â | -0.65 | -1.97 | â |
| Kharchenko et al. | 2013 | 337.567 | 57.195 | â | -2.58 | -2.25 | -60.8 |
| Gozha et al. | 2012 | 337.65 | 57.21 | â | â | â | â |
| Kharchenko et al. | 2012 | 337.567 | 57.195 | â | -2.58 | -2.25 | -60.8 |
| Piskunov et al. | 2008 | 337.64 | 57.207 | â | â | â | â |
| Kharchenko et al. | 2007 | 337.65 | 57.21 | â | 0.3 | â | -60.8 |
| Kharchenko et al. | 2005 | 337.65 | 57.21 | â | -2.99 | -1.54 | -60.79 |
| Dias et al. | 2002 | 337.65 | 57.21 | â | -0.65 | -1.97 | -60.8 |
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 | 25 | â | 255 | â | â |
| Kharchenko et al. | 2016 | 1.50 | 2.05 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.50 | 2.05 | â | 25 | â | â | â | â |
| Gozha et al. | 2012 | 2.50 | â | â | 12 | â | 13804 | â | â |
| Kharchenko et al. | 2012 | 1.50 | 2.05 | â | 25 | â | â | â | â |
| Piskunov et al. | 2008 | 2.50 | 1.92 | â | 12 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.50 | 1.92 | â | 12 | â | â | â | â |
| Dias et al. | 2002 | 2.50 | 1.92 | â | 12 | â | â | â | â |
