Dutra Bica 58

(MWSC 2677)

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0.20 UTI
0.0
CN
0.12
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Dutra Bica 58 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a low-mass, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.31 kpc) differs significantly from the median photometric distance (~1.18 kpc).

Note: This object shares a small percentage of members with a later reported entry. 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.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 266.27 -28.885 0.434 -0.561 -1.615 -34.58
Just et al. 2023 266.259 -28.849 – – – –
Kharchenko et al. 2016 266.259 -28.849 – – – –
Kharchenko et al. 2013 266.268 -28.848 – 1.3 0.0 -15.5
Dias et al. 2002 266.25 -28.86 – 1.3 0.0 -15.5

💡 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– 1.18 6.13 – 1 – 13 – –
Just et al. 2023 – – – 1 – 13 – –
Kharchenko et al. 2016 1.18 6.13 – 1 – – – –
Kharchenko et al. 2013 1.18 6.13 – 1 – – – –
Dias et al. 2002 1.18 6.13 – 1 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Nuclear Star 20.0 266.44 -29.0 0.42 -0.25 -1.4 -15.76 0.25

💡 Note: The % column shows the percentage of members that Dutra Bica 58 shares with each listed object.

Visualization

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