BDSB 97

(BDS2003 97)

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0.32 UTI
0.3
CN
1.0
Cdens
0.38
CC3
0.0
Clit
0.97
Cdup
Stellar density (N50/rad) 8.6 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.97 Unique

Overview

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BDSB 97 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

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

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster, presence of emission related to PAH or warm dust.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 260.005 -35.958 0.593 -0.294 -2.237 71.955
Morales et al. 2013 260.012 -35.972 – – – –

💡 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– 1.74 – – – – – – –
Morales et al. 2013 1.74 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
NGC 6334 IV 63.3 260.05 -35.91 0.59 -0.05 -1.9 -14.06 0.42
NGC 6334 V 46.7 259.99 -35.96 0.54 -0.15 -1.71 -55.76 0.32
BDSB 98 36.7 260.0 -35.93 0.56 -0.19 -1.82 -14.06 0.33
NGC 6334 3.3 260.04 -36.05 0.56 0.15 -1.75 -29.57 0.56
NGC 6334 III 3.3 260.09 -35.9 0.58 -0.24 -1.71 – 0.23

💡 Note: The % column shows the percentage of members that BDSB 97 shares with each listed object.

Visualization

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