Bochum 15
0.24
UTI
0.34
CN
0.1
Cdens
0.25
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
34
Core radius and density
2.5 [pc], 0.5 [pc-2]
- CN 0.34 Poorly populated
- Cdens 0.1 Very loose
- CC3 0.25 Low quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
Bochum 15 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with 3 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 | 115.079 | -33.566 | 0.258 | -2.245 | 3.041 | â |
| Hunt & Reffert | 2024 | 115.072 | -33.551 | 0.257 | -2.23 | 3.043 | 64.423 |
| Cavallo et al. | 2024 | 115.01 | -33.602 | 0.258 | â | â | â |
| Hunt & Reffert | 2023 | 115.072 | -33.551 | 0.257 | -2.23 | 3.043 | 64.423 |
| Loktin & Popova | 2017 | 115.035 | -33.569 | â | -3.737 | 4.906 | â |
| Dias et al. | 2014 | 115.025 | -33.533 | â | -1.06 | 3.49 | â |
| Bukowiecki et al. | 2011 | 115.067 | -33.545 | â | â | â | â |
| van den Bergh | 2006 | 115.025 | -33.55 | â | â | â | â |
| Dias et al. | 2002 | 115.025 | -33.533 | â | -0.87 | 3.09 | â |
| Lynga | 1987 | 115.015 | -33.552 | 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 | 3.12 | 1.58 | 2.22 | 8 | 0.630 | 457 | â | â |
| Hunt & Reffert | 2024 | 3.68 | 1.58 | 2.22 | 59 | â | 310(1) | â | â |
| Cavallo et al. | 2024 | 3.21 | 1.31 | â | 145 | 0.630 | â | â | â |
| Hunt & Reffert | 2023 | 3.68 | 1.58 | 2.22 | 59 | â | â | â | â |
| Loktin & Popova | 2017 | 2.81 | 1.81 | â | 6 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 604 | â | â |
| Bukowiecki et al. | 2011 | 3.12(1) | 1.58 | â | 10 | â | â | â | â |
| van den Bergh | 2006 | 2.81 | 1.83 | â | 5 | â | â | â | â |
| Dias et al. | 2002 | 2.81 | 1.82 | â | 6 | â | â | â | â |
| Lynga | 1987 | â | â | â | 1 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.44 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.44 (50th percentile).