Bochum 5
0.22
UTI
0.0
CN
0.01
Cdens
0.25
CC3
0.42
Clit
1.0
Cdup
Nm (P>50%)
17
Core radius and density
3.6 [pc], 0.07 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.25 Low quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
Bochum 5 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.55 kpc) differs significantly from the median photometric distance (~1.77 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 112.741 | -16.913 | 0.282 | -1.435 | 1.456 | â |
| Richer et al. | 2021 | 112.861 | -17.104 | 0.776 | -2.984 | 1.875 | â |
| Dias et al. | 2018 | â | â | â | -2.34 | 1.28 | â |
| Loktin & Popova | 2017 | 112.8 | -16.965 | â | -1.229 | 5.226 | 38.6 |
| Sampedro et al. | 2017 | 112.75 | -16.933 | â | -0.98 | 1.27 | â |
| Joshi et al. | 2016 | 112.77 | -16.915 | â | â | â | â |
| Dias et al. | 2014 | 112.75 | -16.933 | â | -1.19 | 1.27 | â |
| Gozha et al. | 2012 | 112.75 | -16.933 | â | â | â | â |
| Bukowiecki et al. | 2011 | 112.8 | -16.97 | â | â | â | â |
| Piskunov et al. | 2008 | 112.748 | -16.93 | â | â | â | â |
| Kharchenko et al. | 2007 | 112.75 | -16.93 | â | 0.22 | â | 41.0 |
| van den Bergh | 2006 | 112.75 | -16.933 | â | â | â | â |
| Kharchenko et al. | 2005 | 112.75 | -16.93 | â | -2.11 | -0.66 | 41.0 |
| Dias et al. | 2002 | 112.75 | -16.933 | â | -2.67 | 1.43 | 16.0 |
| Lynga | 1987 | 112.735 | -17.073 | 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 | 1.77 | 0.945 | â | 35 | -0.171 | 1820 | â | â |
| Richer et al. | 2021 | â | 0.33 | â | 350 | â | â | â | â |
| Loktin & Popova | 2017 | 0.90 | 0.63 | â | 38 | â | â | â | â |
| Joshi et al. | 2016 | 1.77 | 1.31 | â | 25 | â | 1820 | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 234 | â | â |
| Gozha et al. | 2012 | 0.87 | â | â | 35 | â | 1820 | â | â |
| Bukowiecki et al. | 2011 | 2.10(1) | 1.83 | â | 18 | â | â | â | â |
| Piskunov et al. | 2008 | 2.00 | 1.26 | â | 282 | â | â | â | â |
| van den Bergh | 2006 | 0.87 | 0.60 | â | 35 | â | â | â | â |
| Kharchenko et al. | 2005 | 2.00 | 1.26 | â | 282 | â | â | â | â |
| Dias et al. | 2002 | 0.87 | 0.61 | â | 35 | -0.171 | â | â | â |
| Lynga | 1987 | 2.29 | â | â | 1 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Richer et al. (2021)
The expected number of WDs is 11.6, 0 WD candidates found, and 0 WD candidates found in the wide search.