Collinder 234

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0.14 UTI
0.0
CN
0.18
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.6 [pc], 0.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Collinder 234 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 24 years.

Note: This object shares a large percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

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.

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Dias et al. (2016)
Part of Tr 16 (Archinal, B. A. & Hynes, S. J. 2003); cat V3.5 (Jan 2016)

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 161.274 -59.713 0.389 -7.15 2.676 -62.383
Dias et al. 2002 161.338 -59.75 – – – –
Alter et al. 1970 161.321 -59.745 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Trumpler 16 76.0 161.26 -59.72 0.4 -6.89 2.59 -0.07 0.93

💡 Note: The % column shows the percentage of members that Collinder 234 shares with each listed object.

Visualization

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