ASCC 33
(MWSC 1077)
0.27
UTI
0.0
CN
0.1
Cdens
0.25
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
0.5 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
ASCC 33 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very close* distance, near the mid-plane, affected by low extinction. It is catalogued as a very massive, near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~0.43 kpc) differs significantly from the median photometric distance (~0.80 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 105.204 | -24.442 | 2.321 | -9.887 | 1.192 | 17.282 |
| Cavallo et al. | 2024 | 104.696 | -24.009 | 2.358 | â | â | â |
| Hunt & Reffert | 2023 | 105.454 | -24.437 | 2.324 | -9.781 | 1.143 | 16.879 |
| Bica et al. | 2019 | 105.797 | -25.054 | â | â | â | â |
| Dias et al. | 2014 | 105.796 | -25.05 | â | -1.86 | 0.22 | â |
| Gozha et al. | 2012 | 105.796 | -25.05 | â | â | â | â |
| Piskunov et al. | 2008 | 105.792 | -25.045 | â | â | â | â |
| Kharchenko et al. | 2007 | 105.79 | -25.05 | â | 0.9 | â | 15.0 |
| Kharchenko et al. | 2005 | 105.79 | -25.05 | â | -3.78 | 3.78 | 15.0 |
| Dias et al. | 2002 | 105.796 | -25.05 | â | -3.78 | 3.78 | 16.15 |
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 | 0.8 | 0.16 | 0.37 | 18 | -0.018 | 7762 | â | â |
| Cavallo et al. | 2024 | 0.43 | 0.44 | â | 89 | 0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.41 | 0.06 | 0.37 | 215 | â | â | â | â |
| Gozha et al. | 2012 | 0.80 | â | â | 18 | â | 7762 | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.16 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.16 | â | 18 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.16 | â | 18 | -0.166 | â | â | â |
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.