ASCC 7
(MWSC 156)
0.30
UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.69
Clit
1.0
Cdup
Stellar density (N50/rad)
0.1 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.12 Very low quality
- Clit 0.69 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 7 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~6.51 kpc) differs significantly from the median photometric distance (~2.00 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 29.721 | 58.941 | 0.154 | -1.391 | 0.174 | -60.797 |
| He et al. | 2023 | 29.62 | 59.266 | 0.411 | -1.447 | -0.856 | -48.91 |
| Just et al. | 2023 | 29.764 | 58.922 | â | â | â | â |
| Bica et al. | 2019 | 29.718 | 58.97 | â | â | â | â |
| Kharchenko et al. | 2016 | 29.764 | 58.922 | â | â | â | â |
| Dias et al. | 2014 | 29.729 | 58.97 | â | 0.24 | -0.98 | â |
| Kharchenko et al. | 2013 | 29.775 | 58.925 | â | 1.94 | -1.21 | -49.0 |
| Gozha et al. | 2012 | 29.729 | 58.97 | â | â | â | â |
| Kharchenko et al. | 2012 | 29.775 | 58.925 | â | 1.94 | -1.21 | -49.0 |
| Piskunov et al. | 2008 | 29.718 | 58.97 | â | â | â | â |
| Kharchenko et al. | 2007 | 29.73 | 58.97 | â | 0.25 | â | -49.0 |
| Kharchenko et al. | 2005 | 29.73 | 58.97 | â | -0.57 | -3.08 | -49.0 |
| Dias et al. | 2002 | 29.729 | 58.97 | â | 0.24 | -0.98 | -49.0 |
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 | 2.0 | 1.55 | â | 25 | â | 1616 | â | â |
| He et al. | 2023 | 2.24 | 1.55 | â | 32 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 25 | â | 282 | â | â |
| Kharchenko et al. | 2016 | 2.00 | 1.40 | â | 25 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.00 | 1.40 | â | 25 | â | â | â | â |
| Gozha et al. | 2012 | 2.00 | â | â | 23 | â | 2951 | â | â |
| Kharchenko et al. | 2012 | 2.00 | 1.40 | â | 25 | â | â | â | â |
| Piskunov et al. | 2008 | 2.00 | 1.55 | â | 23 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.00 | 1.55 | â | 23 | â | â | â | â |
| Dias et al. | 2002 | 2.00 | 1.55 | â | 23 | â | â | â | â |
MOCA
