ASCC 43
(MWSC 1374)
0.24
UTI
0.0
CN
0.06
Cdens
0.0
CC3
0.56
Clit
1.0
Cdup
Stellar density (N50/rad)
0.3 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.0 Very low quality
- Clit 0.56 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 43 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 low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.39 kpc) differs significantly from the median photometric distance (~1.00 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 118.252 | -28.179 | 0.295 | -4.104 | 4.299 | â |
| Just et al. | 2023 | 118.262 | -28.172 | â | â | â | â |
| Bica et al. | 2019 | 118.282 | -28.171 | â | â | â | â |
| Kharchenko et al. | 2016 | 118.262 | -28.172 | â | â | â | â |
| Dias et al. | 2014 | 118.275 | -28.17 | â | -2.95 | 1.29 | â |
| Kharchenko et al. | 2013 | 118.267 | -28.175 | â | -3.45 | 0.95 | 90.5 |
| Gozha et al. | 2012 | 118.275 | -28.17 | â | â | â | â |
| Piskunov et al. | 2008 | 118.266 | -28.168 | â | â | â | â |
| Kharchenko et al. | 2007 | 118.27 | -28.17 | â | 0.35 | â | 90.5 |
| Kharchenko et al. | 2005 | 118.27 | -28.17 | â | -4.4 | 0.47 | â |
| Dias et al. | 2002 | 118.275 | -28.17 | â | -4.4 | 0.47 | 90.5 |
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 | 1.0 | 0.31 | â | 191 | â | 400 | â | â |
| Just et al. | 2023 | â | â | â | 164 | â | 76 | â | â |
| Kharchenko et al. | 2016 | 1.00 | 0.19 | â | 164 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.00 | 0.19 | â | 164 | â | â | â | â |
| Gozha et al. | 2012 | 1.00 | â | â | 191 | â | 724 | â | â |
| Piskunov et al. | 2008 | 1.00 | 0.31 | â | 191 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.00 | 0.31 | â | 191 | â | â | â | â |
| Dias et al. | 2002 | 1.00 | 0.31 | â | 191 | â | â | â | â |
MOCA
