BDSB 125

(MWSC 2990)

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0.19 UTI
0.53
CN
0.14
Cdens
0.38
CC3
0.0
Clit
0.89
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.14 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.89 Very likely unique

Overview

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BDSB 125 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by very high extinction. It is catalogued as a very massive, very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~4.10 kpc) differs significantly from the median photometric distance (~6.70 kpc).

Note: This is very likely a unique object, which shares a small 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=0.89) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant Very high extinction Very massive Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 281.465 -2.729 0.244 -1.172 -3.72 28.108
Just et al. 2023 281.51 -2.657 – – – –
Kharchenko et al. 2016 281.51 -2.657 – – – –
Kharchenko et al. 2013 281.517 -2.655 – 1.29 -8.99 83.3

💡 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] Bfr BSS
Just et al. 2023 – – – 1 – 7780 – –
Kharchenko et al. 2016 6.70 6.45 – 1 – – – –
Kharchenko et al. 2013 6.70 6.45 – 1 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 11 10.7 281.66 -2.77 0.18 -1.14 -3.82 – 0.03
CWNU 3930 1.8 281.31 -2.8 0.21 -1.52 -3.85 47.3 0.17
Ryu 912 1.8 281.32 -2.8 0.19 -1.54 -3.86 – 0.39

💡 Note: The % column shows the percentage of members that BDSB 125 shares with each listed object.

Visualization

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