DBSB 158

(DBS2003 158; MWSC 2363)

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0.15 UTI
0.0
CN
0.13
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.13 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
DBSB 158 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

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 emission related to PAH or warm dust.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 242.845 -51.496 0.346 -2.53 -3.423 -16.615
Just et al. 2023 242.786 -51.525 – – – –
Kharchenko et al. 2016 242.786 -51.525 – – – –
Kharchenko et al. 2013 242.797 -51.525 – -9.83 2.4 –
Morales et al. 2013 242.771 -51.517 – – – –

💡 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– 2.43 2.58 – 507 – 931 – –
Just et al. 2023 – – – 507 – 931 – –
Kharchenko et al. 2016 2.43 2.58 – 507 – – – –
Kharchenko et al. 2013 2.43 2.58 – 507 – – – –
Morales et al. 2013 5.55 – – – – – – –

Visualization

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