DBSB 160

(DBS2003 160)

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0.05 UTI
0.0
CN
0.15
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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DBSB 160 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

Note: This object shares a significant 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.

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of an IR bubble.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 244.185 -50.804 0.355 -3.551 -3.873 -68.52
Morales et al. 2013 244.233 -50.791 – – – –

💡 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– 3.49 – – 3 – – – –
Morales et al. 2013 3.49 – – 3 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
DBSB 161 64.0 244.24 -50.81 0.35 -3.56 -3.89 -68.52 0.18

💡 Note: The % column shows the percentage of members that DBSB 160 shares with each listed object.

Visualization

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