Sh2-287C
(MWSC 1052)
0.12
UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
23
Core radius and density
1.1 [pc], 1.0 [pc-2]
- CN 0.0 Sparse
- Cdens 0.21 Very loose
- CC3 0.25 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Sh2-287C is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~2.22 kpc) differs significantly from the median photometric distance (~3.34 kpc).
Note: This object shares a significant percentage of members with 4 later reported entries. 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 | 104.85 | -4.703 | 0.45 | -1.608 | 0.763 | 48.19 |
| Just et al. | 2023 | 104.896 | -4.665 | â | â | â | â |
| Kharchenko et al. | 2016 | 104.896 | -4.665 | â | â | â | â |
| Kharchenko et al. | 2013 | 104.902 | -4.667 | â | -0.01 | 1.96 | â |
| Bica et al. | 2003 | 104.899 | -4.673 | â | â | â | 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 | 3.34 | 3.61 | â | 8 | â | 41 | â | â |
| Just et al. | 2023 | â | â | â | 8 | â | 41 | â | â |
| Kharchenko et al. | 2016 | 3.34 | 3.61 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.34 | 3.61 | â | 8 | â | â | â | â |
MOCA

Bica et al. (2003)
Classified as infrared cluster (IRC).