BDSB 90

(MWSC 1053)

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0.21 UTI
0.0
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.76
Cdup
Stellar density (N50/rad) 9.9 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.76 Very likely unique

Overview

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BDSB 90 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

Note: This is very likely a unique object, which shares a small 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=0.76) 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– 104.887 -4.812 0.438 -1.488 0.611 62.256
Just et al. 2023 104.903 -4.858 – – – –
Kharchenko et al. 2016 104.903 -4.858 – – – –
Kharchenko et al. 2013 104.91 -4.86 – 0.85 -0.34 41.0

💡 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– 2.66 2.65 – 16 – 150 – –
Just et al. 2023 – – – 16 – 150 – –
Kharchenko et al. 2016 2.66 2.65 – 16 – – – –
Kharchenko et al. 2013 2.66 2.65 – 16 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1723 28.0 104.85 -4.74 0.43 -1.49 0.69 62.26 0.08
S 287 C 24.0 104.88 -4.74 0.44 -1.46 0.6 62.26 0.23
Sh2 287C 8.0 104.85 -4.7 0.45 -1.61 0.76 48.19 0.09

💡 Note: The % column shows the percentage of members that BDSB 90 shares with each listed object.

Visualization

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