Bochum 9
(MWSC 1825)
0.25
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
6.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
Bochum 9 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by low extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.81 kpc) differs significantly from the median photometric distance (~0.94 kpc).
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.
Close
Low extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 158.872 | -60.15 | 0.208 | -5.421 | 2.569 | -0.826 |
| Just et al. | 2023 | 158.92 | -60.126 | â | â | â | â |
| Kharchenko et al. | 2016 | 158.92 | -60.126 | â | â | â | â |
| Dias et al. | 2014 | 158.942 | -60.117 | â | -6.38 | -2.51 | -9.82 |
| Kharchenko et al. | 2013 | 158.925 | -60.13 | â | -10.2 | -0.23 | â |
| Piskunov et al. | 2008 | 158.934 | -60.115 | â | â | â | â |
| van den Bergh | 2006 | 158.94 | -60.126 | â | â | â | â |
| Kharchenko et al. | 2005 | 158.94 | -60.12 | â | -10.46 | 1.34 | â |
| Kharchenko et al. | 2003 | 158.95 | -60.12 | â | -8.98 | 0.36 | â |
| Dias et al. | 2002 | 158.942 | -60.117 | â | -6.38 | -2.51 | -9.82 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 123 | â | 28 | â | â |
| Kharchenko et al. | 2016 | 0.94 | 0.34 | â | 123 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.94 | 0.34 | â | 123 | â | â | â | â |
| Piskunov et al. | 2008 | 0.71 | 0.34 | â | 240 | â | â | â | â |
| van den Bergh | 2006 | 4.60 | 1.95 | â | â | â | â | â | â |
| Kharchenko et al. | 2005 | 0.71 | 0.34 | â | 240 | â | â | â | â |
| Kharchenko et al. | 2003 | 4.60 | 1.95 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.71 | 0.34 | â | 240 | â | â | â | â |
