ASCC 75
(MWSC 2163)
0.40
UTI
0.0
CN
0.18
Cdens
0.25
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
7.8 [arcmin]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.25 Low quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 75 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 near-solar metallicity, very 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 significant percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate 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 | 206.888 | -62.448 | 0.455 | -2.6 | -2.168 | â |
| Hu & Soubiran | 2025 | 206.901 | -62.471 | â | â | â | â |
| Hunt & Reffert | 2024 | 206.932 | -62.452 | 0.476 | -2.632 | -2.187 | â |
| Cavallo et al. | 2024 | 206.901 | -62.471 | 0.474 | â | â | â |
| Hunt & Reffert | 2023 | 206.932 | -62.452 | 0.476 | -2.632 | -2.187 | â |
| Just et al. | 2023 | 206.8 | -62.397 | â | â | â | â |
| Bica et al. | 2019 | 206.785 | -62.418 | â | â | â | â |
| Kharchenko et al. | 2016 | 206.8 | -62.397 | â | â | â | â |
| Dias et al. | 2014 | 206.792 | -62.42 | â | -4.35 | -6.64 | â |
| Kharchenko et al. | 2013 | 206.812 | -62.4 | â | -4.7 | -1.15 | -15.0 |
| Gozha et al. | 2012 | 206.792 | -62.42 | â | â | â | â |
| Piskunov et al. | 2008 | 206.786 | -62.418 | â | â | â | â |
| Kharchenko et al. | 2007 | 206.79 | -62.42 | â | 0.17 | â | -15.0 |
| Kharchenko et al. | 2005 | 206.79 | -62.42 | â | -3.97 | -1.44 | -15.0 |
| Dias et al. | 2002 | 206.792 | -62.42 | â | -4.35 | -6.64 | -38.17 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.160* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 102* | â | â |
| Cavallo et al. | 2024 | 1.69 | 1.56 | â | 759 | -0.330 | â | â | â |
| Hunt & Reffert | 2023 | 1.97 | 1.55 | 1.40 | 103 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 4 | â | 327 | â | â |
| Kharchenko et al. | 2016 | 2.95 | 1.29 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.95 | 1.29 | â | 4 | â | â | â | â |
| Gozha et al. | 2012 | 3.00 | â | â | 4 | â | 9120 | â | â |
| Piskunov et al. | 2008 | 3.00 | 0.93 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2005 | 3.00 | 0.93 | â | 4 | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 0.93 | â | 4 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.