DBSB 85

(MWSC 2104)

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0.20 UTI
0.35
CN
0.45
Cdens
0.25
CC3
0.0
Clit
0.97
Cdup
Radius (P>50% members) 5.1 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.45 Loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.97 Unique

Overview

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DBSB 85 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~2.65 kpc) differs significantly from the median photometric distance (~2.02 kpc).

Note: This is a unique object, which shares a very 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=0.97) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Low mass Young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 199.648 -62.666 0.377 -4.498 -1.875 -38.194
Just et al. 2023 199.6 -62.662 – – – –
Kharchenko et al. 2016 199.6 -62.662 – – – –
Kharchenko et al. 2013 199.612 -62.665 – -15.7 2.0 –

💡 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 – – – 28 – 46 – –
Kharchenko et al. 2016 2.02 4.52 – 28 – – – –
Kharchenko et al. 2013 2.02 4.52 – 28 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2576 25.7 199.65 -62.57 0.49 -4.3 -1.74 -29.39 0.27
UBC 526 2.9 199.68 -62.54 0.49 -4.16 -1.81 -37.02 0.45
VVV 024 2.9 199.65 -62.74 0.38 -4.89 -1.58 – 0.05

💡 Note: The % column shows the percentage of members that DBSB 85 shares with each listed object.

Visualization

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