ASCC 62
(MWSC 1859)
0.56
UTI
0.0
CN
0.57
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.57 Moderately dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 62 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (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
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 162.769 | -60.044 | 0.4 | -6.383 | 2.087 | â |
| Hunt & Reffert | 2024 | 162.762 | -60.083 | 0.404 | -6.394 | 2.087 | 41.383 |
| Cavallo et al. | 2024 | 162.607 | -59.963 | 0.404 | â | â | â |
| Hunt & Reffert | 2023 | 162.762 | -60.083 | 0.404 | -6.394 | 2.087 | 41.383 |
| Just et al. | 2023 | 162.758 | -60.082 | â | â | â | â |
| Bica et al. | 2019 | 162.732 | -60.097 | â | â | â | â |
| Kharchenko et al. | 2016 | 162.758 | -60.082 | â | â | â | â |
| Dias et al. | 2014 | 162.721 | -60.1 | â | -4.23 | -1.38 | â |
| Kharchenko et al. | 2013 | 162.765 | -60.085 | â | -8.64 | 1.45 | -4.0 |
| Gozha et al. | 2012 | 162.721 | -60.1 | â | â | â | â |
| Piskunov et al. | 2008 | 162.714 | -60.092 | â | â | â | â |
| Kharchenko et al. | 2007 | 162.72 | -60.1 | â | 0.28 | â | -4.05 |
| Kharchenko et al. | 2005 | 162.72 | -60.1 | â | -8.72 | 1.68 | -4.05 |
| Dias et al. | 2002 | 162.721 | -60.1 | â | -4.23 | -1.38 | 0.63 |
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 | 174* | â | â |
| Cavallo et al. | 2024 | 2.37 | 0.85 | â | 240 | 0.340 | â | â | â |
| Hunt & Reffert | 2023 | 2.26 | 0.91 | 1.24 | 34 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 10 | â | 532 | â | â |
| Kharchenko et al. | 2016 | 2.32 | 1.65 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.32 | 1.65 | â | 10 | â | â | â | â |
| Gozha et al. | 2012 | 3.00 | â | â | 32 | â | 26915 | â | â |
| Piskunov et al. | 2008 | 3.00 | 0.74 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2005 | 3.00 | 0.74 | â | 32 | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 0.74 | â | 32 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.