ASCC 5
(MWSC 93)
0.73
UTI
0.31
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
3.2 [arcmin]
- CN 0.31 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 5 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 14.462 | 55.848 | 0.562 | -2.401 | -1.897 | -33.138 |
| Hunt & Reffert | 2024 | 14.469 | 55.829 | 0.538 | -2.407 | -1.919 | â |
| Cavallo et al. | 2024 | 14.504 | 55.858 | 0.533 | â | â | â |
| Hunt & Reffert | 2023 | 14.469 | 55.829 | 0.538 | -2.407 | -1.919 | â |
| Just et al. | 2023 | 14.398 | 55.851 | â | â | â | â |
| Bica et al. | 2019 | 14.482 | 55.84 | â | â | â | â |
| Kharchenko et al. | 2016 | 14.398 | 55.851 | â | â | â | â |
| Dias et al. | 2014 | 14.492 | 55.84 | â | -0.2 | -1.83 | â |
| Kharchenko et al. | 2013 | 14.407 | 55.855 | â | -1.82 | -3.15 | -43.0 |
| Gozha et al. | 2012 | 14.492 | 55.84 | â | â | â | â |
| Kharchenko et al. | 2012 | 14.407 | 55.855 | â | -1.82 | -3.15 | -43.0 |
| Piskunov et al. | 2008 | 14.482 | 55.84 | â | â | â | â |
| Kharchenko et al. | 2007 | 14.49 | 55.84 | â | 0.13 | â | -43.0 |
| Kharchenko et al. | 2005 | 14.49 | 55.84 | â | -3.1 | -2.91 | -43.0 |
| Dias et al. | 2002 | 14.492 | 55.84 | â | -0.2 | -1.83 | -43.0 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 173* | â | â |
| Cavallo et al. | 2024 | 1.86 | 0.86 | â | 15 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 1.75 | 1.18 | 0.72 | 21 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 60 | â | 8 | â | â |
| Kharchenko et al. | 2016 | 0.52 | 0.07 | â | 60 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.52 | 0.07 | â | 60 | â | â | â | â |
| Gozha et al. | 2012 | 1.50 | â | â | 11 | â | 155 | â | â |
| Kharchenko et al. | 2012 | 0.52 | 0.07 | â | 60 | â | â | â | â |
| Piskunov et al. | 2008 | 1.50 | 0.78 | â | 11 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.50 | 0.78 | â | 11 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 0.78 | â | 11 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.