BDB2003 G333.60-00.21

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0.02 UTI
0.0
CN
0.04
Cdens
0.25
CC3
0.0
Clit
0.32
Cdup
Core radius and density 2.6 [pc], 0.2 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.04 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.32 Possibly duplicate

Overview

â„šī¸
BDB2003 G333.60-00.21 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.32) 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– 245.6 -50.122 0.35 -2.739 -4.011 -29.655
Morales et al. 2013 245.542 -50.097 – – – –

💡 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 – – – – – – –
Morales et al. 2013 3.49 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
G333.6-0.2 68.0 245.61 -50.11 0.36 -2.73 -4.01 -14.28 0.03
UBC 543 20.0 245.73 -50.18 0.39 -2.36 -4.12 -71.96 0.1
CWWDL 13867 12.0 245.73 -50.18 0.41 -2.41 -4.1 -72.39 0.04
FoF 273 12.0 245.72 -50.18 0.39 -2.35 -4.12 -72.39 0.61
CWWDL 1589 8.0 245.73 -50.17 0.39 -2.36 -4.12 -71.96 0.0
DBSB 165 4.0 245.43 -50.42 0.4 -2.77 -4.11 -33.85 0.05

💡 Note: The % column shows the percentage of members that BDB2003 G333.60-00.21 shares with each listed object.

Visualization

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