Sh2-235
(MWSC 629)
0.18
UTI
0.0
CN
0.06
Cdens
0.62
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
19
Core radius and density
1.5 [pc], 0.3 [pc-2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Sh2-235 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a small percentage of members with at least one entry reported in the same catalogue. 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 | 85.217 | 35.887 | 0.587 | 0.297 | -2.972 | â |
| Just et al. | 2023 | 85.168 | 35.921 | â | â | â | â |
| Kharchenko et al. | 2016 | 85.168 | 35.921 | â | â | â | â |
| Kharchenko et al. | 2013 | 85.177 | 35.92 | â | 2.11 | -3.43 | â |
| Kharchenko et al. | 2012 | 85.177 | 35.92 | â | 3.27 | -3.93 | â |
| Bica et al. | 2003 | 85.282 | 35.831 | 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 | 2.31 | 3.28 | â | 4 | â | 75 | â | â |
| Just et al. | 2023 | â | â | â | 4 | â | 75 | â | â |
| Kharchenko et al. | 2016 | 2.31 | 3.28 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.31 | 3.28 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.10 | 1.26 | â | 1084 | â | â | â | â |
MOCA

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