Collinder 33

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0.12 UTI
0.0
CN
0.09
Cdens
0.12
CC3
0.19
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.19 Rarely studied
  • Cdup 1.0 Unique

Overview

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Collinder 33 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~2.87 kpc) differs significantly from the median photometric distance (~1.05 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 44.897 60.422 0.349 -0.432 -0.681 -46.623
Dib et al. 2018 44.815 60.3 – – – –
Joshi et al. 2016 44.815 60.3 – – – –
Piskunov et al. 2008 44.808 60.395 – – – –
Kharchenko et al. 2007 44.82 60.4 – 0.36 – -6.75
Piskunov et al. 2007 44.808 60.395 – – – –
Kharchenko et al. 2005 44.82 60.4 – 2.7 3.17 -6.75
Kharchenko et al. 2003 44.82 60.4 – 3.62 2.33 –
Lynga 1987 44.835 60.399 – – – –

💡 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 99999– 1.05 1.26 – 229 – 507 – –
Dib et al. 2018 1.10 – – 222 – – – –
Joshi et al. 2016 1.10 1.10 – 222 – 562 – –
Piskunov et al. 2008 1.00 1.26 – 229 – 507(1) – –
Piskunov et al. 2007 1.00 1.26 – 229 – 150 – –
Kharchenko et al. 2005 1.00 1.26 – 229 – – – –
Kharchenko et al. 2003 1.11 1.26 – – – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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