BDSB30

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0.66 UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.4
Clit
1.0
Cdup
Stellar density (N50/rad) 106.6 [N/pc2]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.4 Poorly studied
  • Cdup 1.0 Unique

Overview

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BDSB30 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 333.652 61.443 1.115 -1.537 -3.002 -16.154
Hunt & Reffert 2024 333.663 61.444 1.126 -1.399 -2.868 -15.021
Celli et al. 2024 333.667 61.433 – – – –
Cavallo et al. 2024 333.876 61.476 1.129 – – –
Hunt & Reffert 2023 333.663 61.444 1.126 -1.399 -2.868 -15.021
Cantat-Gaudin et al. 2020 333.667 61.433 1.109 -1.579 -3.005 –
Cantat-Gaudin & Anders 2020 333.667 61.433 1.109 -1.579 -3.005 –
Cantat-Gaudin et al. 2018 333.667 61.433 1.109 -1.579 -3.005 –

💡 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– 0.88 2.975 2.6 8 -0.360 156 – –
Hunt & Reffert 2024 – – – – – 269(1) – –
Celli et al. 2024 – – – 4 – 43 – –
Cavallo et al. 2024 1.47 2.87 – 10 -0.360 – – –
Hunt & Reffert 2023 0.87 3.08 2.60 8 – – – –
Cantat-Gaudin & Anders 2020 0.88 – – – – – – –
Cantat-Gaudin et al. 2018 0.88 – – – – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0181 2.0 334.02 61.12 1.13 -1.0 -3.01 -15.42 0.23

💡 Note: The % column shows the percentage of members that BDSB30 shares with each listed object.

Visualization

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