DBSB 96

(DBS2003 96; DBSB 95; DBS2003 95)

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0.13 UTI
0.39
CN
0.27
Cdens
0.75
CC3
0.0
Clit
0.46
Cdup
Stellar density (N50/rad) 1.3 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.27 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.46 Possibly duplicate

Overview

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DBSB 96 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, 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– 236.086 -54.222 0.415 -3.733 -3.193 -25.174
Morales et al. 2013 236.188 -54.111 – – – –

💡 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– 2.67 – – 2 – – – –
Morales et al. 2013 2.67 – – 2 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 62 53.8 236.09 -54.22 0.42 -3.77 -3.11 -32.08 0.13
HSC 2728 35.9 235.97 -54.31 0.43 -3.7 -3.19 -33.99 0.17

💡 Note: The % column shows the percentage of members that DBSB 96 shares with each listed object.

Visualization

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