ASCC 40
(MWSC 1266)
0.36
UTI
0.26
CN
0.02
Cdens
0.62
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.1 [N/pc2]
- CN 0.26 Poorly populated
- Cdens 0.02 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
ASCC 40 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~5.51 kpc) differs significantly from the median photometric distance (~0.70 kpc).
Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 113.43 | -13.765 | 0.182 | -1.378 | 1.741 | 95.095 |
| Just et al. | 2023 | 113.408 | -13.763 | â | â | â | â |
| Bica et al. | 2019 | 113.401 | -13.755 | â | â | â | â |
| Kharchenko et al. | 2016 | 113.408 | -13.763 | â | â | â | â |
| Dias et al. | 2014 | 113.4 | -13.76 | â | -2.47 | 1.72 | â |
| Kharchenko et al. | 2013 | 113.415 | -13.765 | â | -1.13 | -1.12 | â |
| Piskunov et al. | 2008 | 113.391 | -13.76 | â | â | â | â |
| Kharchenko et al. | 2005 | 113.4 | -13.76 | â | -2.07 | 2.7 | â |
| Dias et al. | 2002 | 113.4 | -13.76 | â | -2.47 | 1.72 | 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 | 0.7 | 0.34 | â | 506 | â | 630 | â | â |
| Just et al. | 2023 | â | â | â | 631 | â | 630 | â | â |
| Kharchenko et al. | 2016 | 3.11 | 1.29 | â | 631 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.11 | 1.29 | â | 631 | â | â | â | â |
| Piskunov et al. | 2008 | 0.70 | 0.34 | â | 380 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.70 | 0.34 | â | 380 | â | â | â | â |
| Dias et al. | 2002 | 0.70 | 0.34 | â | 380 | â | â | â | â |
MOCA
