Bochum 9

(MWSC 1825)

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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

â„šī¸
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).

âš 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 158.872 -60.15 0.208 -5.421 2.569 -0.826
Just et al. 2023 158.92 -60.126 – – – –
Kharchenko et al. 2016 158.92 -60.126 – – – –
Dias et al. 2014 158.942 -60.117 – -6.38 -2.51 -9.82
Kharchenko et al. 2013 158.925 -60.13 – -10.2 -0.23 –
Piskunov et al. 2008 158.934 -60.115 – – – –
van den Bergh 2006 158.94 -60.126 – – – –
Kharchenko et al. 2005 158.94 -60.12 – -10.46 1.34 –
Kharchenko et al. 2003 158.95 -60.12 – -8.98 0.36 –
Dias et al. 2002 158.942 -60.117 – -6.38 -2.51 -9.82

💡 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 – – – 123 – 28 – –
Kharchenko et al. 2016 0.94 0.34 – 123 – – – –
Kharchenko et al. 2013 0.94 0.34 – 123 – – – –
Piskunov et al. 2008 0.71 0.34 – 240 – – – –
van den Bergh 2006 4.60 1.95 – – – – – –
Kharchenko et al. 2005 0.71 0.34 – 240 – – – –
Kharchenko et al. 2003 4.60 1.95 – – – – – –
Dias et al. 2002 0.71 0.34 – 240 – – – –

Visualization

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