SAI 1
(MWSC 18)
0.18
UTI
0.0
CN
0.03
Cdens
0.38
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
22
Core radius and density
4.6 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.38 Low quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
SAI 1 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.69 kpc) differs significantly from the median photometric distance (~1.91 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 | 2.126 | 51.729 | 0.271 | -2.669 | -1.223 | â |
| Just et al. | 2023 | 2.103 | 51.721 | â | â | â | â |
| Bica et al. | 2019 | 2.09 | 51.725 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -3.99 | -2.31 | â |
| Sampedro et al. | 2017 | 2.083 | 51.721 | â | -4.47 | -1.26 | â |
| Kharchenko et al. | 2016 | 2.103 | 51.721 | â | â | â | â |
| Dias et al. | 2014 | 2.083 | 51.721 | â | 0.66 | -0.84 | â |
| Kharchenko et al. | 2013 | 2.112 | 51.724 | â | -4.2 | -1.78 | â |
| Kharchenko et al. | 2012 | 2.112 | 51.724 | â | -4.2 | -1.78 | â |
| Glushkova et al. | 2010 | 2.085 | 51.721 | â | â | â | â |
| Dias et al. | 2002 | 2.083 | 51.721 | â | 0.31 | -0.88 | 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 | 1.91 | 0.98 | â | 1862 | â | 7 | â | â |
| Just et al. | 2023 | â | â | â | 1862 | â | 7 | â | â |
| Kharchenko et al. | 2016 | 1.91 | 0.98 | â | 1862 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.91 | 0.98 | â | 1862 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.91 | 0.98 | â | 1862 | â | â | â | â |
| Glushkova et al. | 2010 | 2.17 | 1.07 | â | 1259 | â | â | â | â |
| Dias et al. | 2002 | 2.17 | 1.07 | â | 1259 | â | â | â | â |
MOCA
