Desvoivres 2
0.19
UTI
0.0
CN
0.43
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
0.9 [pc], 2.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.43 Loose
- CC3 0.38 Low quality
- Clit 0.06 Rarely studied
- Cdup 1.0 Unique
Overview
Desvoivres 2 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
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 | 99.975 | 6.058 | 0.651 | -1.53 | 0.959 | â |
| Hunt & Reffert | 2024 | 99.98 | 6.037 | 0.641 | -1.518 | 0.944 | â |
| Cavallo et al. | 2024 | 99.951 | 6.071 | 0.65 | â | â | â |
| Hunt & Reffert | 2023 | 99.98 | 6.037 | 0.641 | -1.518 | 0.944 | â |
| Bica et al. | 2019 | 99.999 | 6.0 | 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 | 1.44 | 1.28 | 0.86 | 83 | 0.390 | 89 | â | â |
| Hunt & Reffert | 2024 | 1.44 | 1.28 | 0.86 | 83 | â | 89(1) | â | â |
| Cavallo et al. | 2024 | 1.55 | 1.42 | â | 56 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 1.44 | 1.28 | 0.86 | 83 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G20, along with HSC_1629, NGC_2244, Collinder_107 and Collinder_106.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Bica et al. (2019)
The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.