ASCC 116
(MWSC 3576)
0.34
UTI
0.0
CN
0.07
Cdens
0.25
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
4.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.25 Low quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 116 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very massive, near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
Very distant
Moderate extinction
Very massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 329.67 | 54.495 | 0.194 | -2.874 | -2.513 | â |
| Just et al. | 2023 | 329.62 | 54.487 | â | â | â | â |
| Donor et al. | 2020 | 329.625 | 54.49 | â | -1.4 | -2.03 | -22.5 |
| Bica et al. | 2019 | 329.638 | 54.486 | â | â | â | â |
| Kharchenko et al. | 2016 | 329.62 | 54.487 | â | â | â | â |
| Dias et al. | 2014 | 329.642 | 54.49 | â | -3.44 | -4.05 | â |
| Kharchenko et al. | 2013 | 329.625 | 54.49 | â | -3.5 | -4.5 | -30.6 |
| Gozha et al. | 2012 | 329.642 | 54.49 | â | â | â | â |
| Kharchenko et al. | 2012 | 329.625 | 54.49 | â | -3.5 | -4.5 | -30.6 |
| Piskunov et al. | 2008 | 329.638 | 54.486 | â | â | â | â |
| Kharchenko et al. | 2007 | 329.64 | 54.49 | â | 0.18 | â | -30.6 |
| Kharchenko et al. | 2005 | 329.64 | 54.49 | â | -3.51 | -4.74 | -30.6 |
| Dias et al. | 2002 | 329.642 | 54.49 | â | -3.44 | -4.05 | -30.6 |
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 | 89 | â | 81 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.130 | â | â | â |
| Kharchenko et al. | 2016 | 1.50 | 1.58 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.50 | 1.58 | â | 89 | â | â | â | â |
| Gozha et al. | 2012 | 5.00 | â | â | 11 | â | 16982 | â | â |
| Kharchenko et al. | 2012 | 1.50 | 1.58 | â | 89 | â | â | â | â |
| Piskunov et al. | 2008 | 5.00 | 1.58 | â | 11 | â | â | â | â |
| Kharchenko et al. | 2005 | 5.00 | 1.58 | â | 11 | â | â | â | â |
| Dias et al. | 2002 | 5.00 | 1.58 | â | 11 | â | â | â | â |
