ASCC 100
(MWSC 3038)
0.85
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
5.1 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
ASCC 100 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 285.272 | 32.954 | 2.798 | 1.954 | -3.312 | -16.067 |
| Zhang et al. | 2024 | 285.403 | 33.601 | â | â | â | â |
| Cavallo et al. | 2024 | 284.63 | 32.437 | 2.749 | â | â | â |
| Hunt & Reffert | 2023 | 285.403 | 33.601 | 2.751 | 1.732 | -3.451 | -13.846 |
| Just et al. | 2023 | 285.401 | 33.573 | â | â | â | â |
| Bica et al. | 2019 | 285.409 | 33.571 | â | â | â | â |
| Kharchenko et al. | 2016 | 285.401 | 33.573 | â | â | â | â |
| Dias et al. | 2014 | 285.404 | 33.57 | â | 0.2 | -3.41 | â |
| Kharchenko et al. | 2013 | 285.405 | 33.575 | â | 2.2 | -2.0 | -25.6 |
| Gozha et al. | 2012 | 285.404 | 33.57 | â | â | â | â |
| Piskunov et al. | 2008 | 285.393 | 33.567 | â | â | â | â |
| Kharchenko et al. | 2007 | 285.4 | 33.57 | â | 0.31 | â | -22.9 |
| Kharchenko et al. | 2005 | 285.4 | 33.57 | â | 2.29 | -1.51 | -22.89 |
| Dias et al. | 2002 | 285.404 | 33.57 | â | 2.29 | -1.51 | -25.96 |
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 | 0.35 | 0.07 | 0.66 | 89 | 0.021 | 16 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.017(1) | â | â | â |
| Cavallo et al. | 2024 | 0.37 | 0.46 | â | 16 | 0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.35 | 0.23 | 0.66 | 65 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 89 | â | 12 | â | â |
| Kharchenko et al. | 2016 | 0.35 | 0.07 | â | 89 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.35 | 0.07 | â | 89 | â | â | â | â |
| Gozha et al. | 2012 | 0.35 | â | â | 102 | â | 19 | â | â |
| Piskunov et al. | 2008 | 0.35 | 0.06 | â | 102 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.35 | 0.06 | â | 102 | â | â | â | â |
| Dias et al. | 2002 | 0.35 | 0.06 | â | 102 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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