BDSB 166

(MWSC 2606)

Click to load Aladin Lite
0.13 UTI
0.0
CN
0.54
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 2.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.54 Moderately dense
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
BDSB 166 is a sparse, moderately dense object of very low C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by high extinction. It is catalogued as an extremely massive, very young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~1.61 kpc) differs significantly from the median photometric distance (~6.75 kpc).

Note: This object shares a moderate percentage of members 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=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 262.208 -36.566 0.621 -1.676 -2.807 -10.348
Just et al. 2023 262.235 -36.562 – – – –
Kharchenko et al. 2016 262.235 -36.562 – – – –
Kharchenko et al. 2013 262.245 -36.562 – -2.78 -0.54 –

💡 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– 6.75 3.39 – 1 – 18535 – –
Just et al. 2023 – – – 1 – 18535 – –
Kharchenko et al. 2016 6.75 3.39 – 1 – – – –
Kharchenko et al. 2013 6.75 3.39 – 1 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 165 40.0 262.33 -36.65 0.49 -1.61 -2.54 -19.16 0.27

💡 Note: The % column shows the percentage of members that BDSB 166 shares with each listed object.

Visualization

â„šī¸