Alessi 16
(MWSC 968)
0.23
UTI
0.0
CN
0.26
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.0 Sparse
- Cdens 0.26 Loose
- CC3 0.25 Low quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
Alessi 16 is a sparse, 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 low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.05 kpc) differs significantly from the median photometric distance (~2.09 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
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 | 100.826 | 2.15 | 0.328 | -0.258 | 1.502 | 70.834 |
| Just et al. | 2023 | 100.883 | 2.177 | â | â | â | â |
| Kharchenko et al. | 2016 | 100.883 | 2.177 | â | â | â | â |
| Kharchenko et al. | 2013 | 100.89 | 2.175 | â | -0.98 | -2.14 | 50.3 |
| Kronberger et al. | 2006 | 100.896 | 2.173 | â | â | â | â |
| Dias et al. | 2002 | 100.896 | 2.173 | â | -0.98 | -2.14 | â |
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 | 2.09 | 1.94 | â | 447 | â | 16 | â | â |
| Just et al. | 2023 | â | â | â | 447 | â | 16 | â | â |
| Kharchenko et al. | 2016 | 2.09 | 1.94 | â | 447 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.09 | 1.94 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 1.19 | 0.84 | â | 1122 | â | â | â | â |
