ASCC 126
(MWSC 3699)
0.29
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.61
Clit
1.0
Cdup
Nm (P>50%)
20
Core radius and density
9.5 [pc], 0.04 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.61 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 126 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~5.85 kpc) differs significantly from the median photometric distance (~0.90 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 346.485 | 51.072 | 0.171 | -2.663 | -2.245 | -57.673 |
| Just et al. | 2023 | 346.447 | 51.067 | â | â | â | â |
| Bica et al. | 2019 | 346.564 | 51.052 | â | â | â | â |
| Dib et al. | 2018 | 346.455 | 51.07 | â | â | â | â |
| Sampedro et al. | 2017 | 346.575 | 51.05 | â | -0.44 | -1.06 | â |
| Joshi et al. | 2016 | 346.455 | 51.07 | â | â | â | â |
| Kharchenko et al. | 2016 | 346.447 | 51.067 | â | â | â | â |
| Dias et al. | 2014 | 346.575 | 51.05 | â | -0.49 | -1.58 | â |
| Kharchenko et al. | 2013 | 346.455 | 51.07 | â | -2.02 | -2.97 | -12.7 |
| Gozha et al. | 2012 | 346.575 | 51.05 | â | â | â | â |
| Kharchenko et al. | 2012 | 346.455 | 51.07 | â | -2.02 | -2.97 | -12.7 |
| Piskunov et al. | 2008 | 346.57 | 51.042 | â | â | â | â |
| Kharchenko et al. | 2007 | 346.57 | 51.05 | â | 0.3 | â | -12.7 |
| Kharchenko et al. | 2005 | 346.57 | 51.05 | â | -0.66 | -3.01 | -12.69 |
| Dias et al. | 2002 | 346.575 | 51.05 | â | -0.49 | -1.58 | -12.7 |
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 | 0.9 | 0.32 | â | 28 | â | 324 | â | â |
| Just et al. | 2023 | â | â | â | 28 | â | 92 | â | â |
| Dib et al. | 2018 | 0.90 | â | â | 28 | â | â | â | â |
| Joshi et al. | 2016 | 0.90 | 0.32 | â | 28 | â | 324 | â | â |
| Kharchenko et al. | 2016 | 0.90 | 0.32 | â | 28 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.90 | 0.32 | â | 28 | â | â | â | â |
| Gozha et al. | 2012 | 0.80 | â | â | 18 | â | 324 | â | â |
| Kharchenko et al. | 2012 | 0.90 | 0.32 | â | 28 | â | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.32 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.32 | â | 18 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.32 | â | 18 | â | â | â | â |
MOCA
