BDSB 132

(BDS2003 132)

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0.07 UTI
0.37
CN
0.36
Cdens
0.25
CC3
0.0
Clit
0.35
Cdup
Stellar density (N50/rad) 1.8 [N/pc2]
  • CN 0.37 Poorly populated
  • Cdens 0.36 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.35 Possibly duplicate

Overview

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BDSB 132 is a poorly populated, 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.

(*): The parallax distance estimate (~2.13 kpc) differs significantly from the median photometric distance (~11.40 kpc).

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.35) 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.

Bica et al. (2003)
Classified as stellar group (IRGr).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 287.528 9.095 0.47 -3.054 -5.782 24.454
Morales et al. 2013 287.546 9.117 – – – –
Bica et al. 2003 287.541 9.115 – – – –

💡 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– 11.4 – – – – – – –
Morales et al. 2013 11.40 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
W49A 64.9 287.53 9.08 0.47 -3.04 -5.77 24.45 0.12
W49A Welch Ring 62.2 287.53 9.08 0.47 -3.06 -5.77 24.84 0.01
W49A-southwest 43.2 287.52 9.08 0.43 -3.06 -5.64 45.46 0.12

💡 Note: The % column shows the percentage of members that BDSB 132 shares with each listed object.

Visualization

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