ASCC 8
(MWSC 180)
0.37
UTI
0.0
CN
0.12
Cdens
0.25
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
6.1 [arcmin]
- CN 0.0 Sparse
- Cdens 0.12 Very loose
- CC3 0.25 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 8 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, young cluster (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~3.14 kpc) differs significantly from the median photometric distance (~2.04 kpc).
Relatively close
Moderate extinction
Massive
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 35.055 | 59.616 | 0.318 | -1.51 | -0.669 | -51.364 |
| He et al. | 2023 | 34.408 | 59.231 | 0.91 | 0.992 | -2.444 | â |
| Just et al. | 2023 | 35.178 | 59.687 | â | â | â | â |
| Bica et al. | 2019 | 35.2 | 59.614 | â | â | â | â |
| Loktin & Popova | 2017 | 35.205 | 59.61 | â | 0.482 | -2.286 | -12.9 |
| Kharchenko et al. | 2016 | 35.178 | 59.687 | â | â | â | â |
| Dias et al. | 2014 | 35.204 | 59.61 | â | 0.56 | -0.43 | â |
| Kharchenko et al. | 2013 | 35.19 | 59.69 | â | -0.82 | 0.19 | -12.9 |
| Gozha et al. | 2012 | 35.204 | 59.61 | â | â | â | â |
| Kharchenko et al. | 2012 | 35.19 | 59.69 | â | -0.82 | 0.19 | -12.89 |
| Piskunov et al. | 2008 | 35.193 | 59.605 | â | â | â | â |
| Kharchenko et al. | 2007 | 35.2 | 59.61 | â | 0.3 | â | -42.09 |
| Kharchenko et al. | 2005 | 35.2 | 59.61 | â | -1.24 | 0.57 | -42.09 |
| Dias et al. | 2002 | 35.204 | 59.61 | â | 0.56 | -0.43 | -17.4 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| He et al. | 2023 | 1.12 | 2.40 | â | 50 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 59 | â | 411 | â | â |
| Loktin & Popova | 2017 | 2.04 | 1.43 | â | 79 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.80 | 1.86 | â | 59 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.80 | 1.86 | â | 59 | â | â | â | â |
| Gozha et al. | 2012 | 2.20 | â | â | 6 | â | 9550 | â | â |
| Kharchenko et al. | 2012 | 1.80 | 1.86 | â | 59 | â | â | â | â |
| Piskunov et al. | 2008 | 2.20 | 1.71 | â | 6 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.20 | 1.71 | â | 6 | â | â | â | â |
| Dias et al. | 2002 | 2.20 | 1.71 | â | 6 | â | â | â | â |
