dutra bica 26

(DB2000 26)

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0.05 UTI
0.0
CN
0.1
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
dutra bica 26 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.

(*): The parallax distance estimate (~2.94 kpc) differs significantly from the median photometric distance (~5.90 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.

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully 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– 267.196 -28.037 0.34 -0.85 -3.54 –
Morales et al. 2013 267.173 -28.028 – – – –

💡 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– 5.9 – – 1 – – – –
Morales et al. 2013 5.90 – – 1 – – – –

Visualization

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