BDSB 99

(BDS2003 99)

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0.31 UTI
0.55
CN
0.42
Cdens
0.75
CC3
0.0
Clit
0.92
Cdup
Core radius and density 1.2 [pc], 2.1 [pc-2]
  • CN 0.55 Moderately populated
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.92 Very likely unique

Overview

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BDSB 99 is a moderately populated, loose object of high 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 very likely a unique object, which shares a very 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.

Bica et al. (2019)
Present study.

Morales et al. (2013)
Classified as morphological type 'OC0' (emerging exposed cluster). Morphological flag: possibly associated submm emission surrounding the cluster, presence of an IR bubble.

Bica et al. (2003)
Classified as stellar group (IRGr).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 259.782 -35.72 0.552 -0.054 -1.56 -26.711
Morales et al. 2013 259.746 -35.697 – – – –
Bica et al. 2003 259.75 -35.695 – – – –

💡 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 V 8.5 259.99 -35.96 0.54 -0.15 -1.71 -55.76 0.22
Bochum 13 6.8 259.34 -35.53 0.57 -0.28 -1.26 -62.15 0.9
NGC 6334 IV 6.8 260.05 -35.91 0.59 -0.05 -1.9 -14.06 0.23
BDSB 98 5.1 260.0 -35.93 0.56 -0.19 -1.82 -14.06 0.04
NGC 6334 3.4 260.04 -36.05 0.56 0.15 -1.75 -29.57 0.43
NGC 6334 III 1.7 260.09 -35.9 0.58 -0.24 -1.71 – 0.05

💡 Note: The % column shows the percentage of members that BDSB 99 shares with each listed object.

Visualization

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