ASCC 91
(MWSC 2702)
0.18
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
19
Core radius and density
2.2 [pc], 0.06 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
ASCC 91 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~4.59 kpc) differs significantly from the median photometric distance (~0.86 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 267.244 | -37.391 | 0.218 | -1.967 | -2.581 | 5.932 |
| Just et al. | 2023 | 267.2 | -37.371 | â | â | â | â |
| Bica et al. | 2019 | 267.227 | -37.363 | â | â | â | â |
| Dib et al. | 2018 | 267.21 | -37.37 | â | â | â | â |
| Sampedro et al. | 2017 | 267.225 | -37.36 | â | -1.91 | -4.62 | â |
| Joshi et al. | 2016 | 267.21 | -37.37 | â | â | â | â |
| Kharchenko et al. | 2016 | 267.2 | -37.371 | â | â | â | â |
| Dias et al. | 2014 | 267.225 | -37.36 | â | -1.57 | -4.13 | â |
| Kharchenko et al. | 2013 | 267.21 | -37.37 | â | 2.0 | -4.2 | â |
| Piskunov et al. | 2008 | 267.217 | -37.358 | â | â | â | â |
| Kharchenko et al. | 2005 | 267.22 | -37.36 | â | 2.29 | -4.92 | â |
| Dias et al. | 2002 | 267.225 | -37.36 | â | -1.64 | -4.18 | -14.51 |
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 | 0.86 | 0.325 | â | 447 | -0.035 | 236 | â | â |
| Just et al. | 2023 | â | â | â | 447 | â | 55 | â | â |
| Dib et al. | 2018 | 0.86 | â | â | 447 | â | â | â | â |
| Joshi et al. | 2016 | 0.86 | 0.33 | â | 447 | â | 417 | â | â |
| Kharchenko et al. | 2016 | 0.86 | 0.33 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.86 | 0.33 | â | 447 | -0.035 | â | â | â |
| Piskunov et al. | 2008 | 0.80 | 0.32 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.80 | 0.32 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 0.80 | 0.32 | â | 447 | -0.035 | â | â | â |
MOCA
