BDSB 54

(BDS2003 54)

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0.08 UTI
0.0
CN
0.29
Cdens
0.38
CC3
0.0
Clit
0.64
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.64 Likely unique

Overview

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BDSB 54 is a sparse, loose object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 23 years.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a very small percentage with at least one entry reported in the same catalogue. See table with shared members information.

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 36.394 62.041 0.468 -0.776 -0.546 –
Bica et al. 2003 36.355 62.061 – – – –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
SAI 19 44.0 36.65 62.0 0.48 -0.7 -0.12 -27.12 0.1
IRAS 02232+6138 36.0 36.65 62.0 0.48 -0.68 -0.13 -24.58 0.6
W3-IRS5 36.0 36.41 62.09 0.46 -1.0 -0.53 30.96 0.19
IC1795 2 20.0 36.87 61.94 0.48 -0.71 -0.57 -58.52 0.1
CWNU 3691 16.0 36.65 62.0 0.47 -0.69 -0.06 -21.84 0.02
BDSB 56 4.0 36.53 62.02 0.48 -0.98 -0.11 -21.84 0.14

💡 Note: The % column shows the percentage of members that BDSB 54 shares with each listed object.

Visualization

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