Bochum 2
(MWSC 991)
0.41
UTI
0.0
CN
0.17
Cdens
0.25
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
0.9 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.17 Very loose
- CC3 0.25 Low quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Bochum 2 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~5.36 kpc) differs significantly from the median photometric distance (~2.78 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 102.214 | 0.378 | 0.186 | -0.266 | 0.236 | 84.125 |
| Hunt & Reffert | 2024 | 102.207 | 0.377 | 0.192 | -0.309 | 0.24 | â |
| Cavallo et al. | 2024 | 102.21 | 0.416 | 0.19 | â | â | â |
| Hunt & Reffert | 2023 | 102.207 | 0.377 | 0.192 | -0.309 | 0.24 | â |
| Just et al. | 2023 | 102.203 | 0.382 | â | â | â | â |
| Jaehnig et al. | 2021 | 102.21 | 0.378 | 0.161 | -0.316 | 0.228 | â |
| Loktin & Popova | 2017 | 102.225 | -0.383 | â | -0.05 | -1.68 | 67.0 |
| Kharchenko et al. | 2016 | 102.203 | 0.382 | â | â | â | â |
| Dias et al. | 2014 | 102.225 | 0.383 | â | -0.03 | -1.73 | â |
| Kharchenko et al. | 2013 | 102.21 | 0.38 | â | 1.37 | -3.01 | 67.0 |
| Gozha et al. | 2012 | 102.225 | 0.383 | â | â | â | â |
| Bukowiecki et al. | 2011 | 102.204 | 0.378 | â | â | â | â |
| Kharchenko et al. | 2007 | 102.22 | 0.38 | â | 0.01 | â | â |
| van den Bergh | 2006 | 102.225 | 0.383 | â | â | â | â |
| Dias et al. | 2002 | 102.225 | 0.383 | â | -0.05 | -1.68 | 66.3 |
| Dambis | 1999 | 102.225 | 0.383 | 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 | 2.78 | 2.63 | 2.41 | 5 | 0.110 | 336 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 662(1) | â | â |
| Cavallo et al. | 2024 | 4.94 | 2.77 | â | 52 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 4.48 | 2.62 | 2.41 | 79 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 5 | â | 82 | â | â |
| Jaehnig et al. | 2021 | 6.19(1) | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.97 | 2.63 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.78 | 2.71 | â | 5 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.78 | 2.71 | â | 5 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 336 | â | â |
| Gozha et al. | 2012 | 2.66 | â | â | 5 | â | â | â | â |
| Bukowiecki et al. | 2011 | 2.50(1) | 0.74 | â | 178 | â | â | â | â |
| van den Bergh | 2006 | 2.66 | 2.57 | â | 5 | â | â | â | â |
| Dias et al. | 2002 | 2.66 | 2.58 | â | 5 | â | â | â | â |
| Dambis | 1999 | 6.43 | 2.77 | â | 3 | 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)
Gold sample.