DBSB 21

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0.54 UTI
0.33
CN
1.0
Cdens
0.5
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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DBSB 21 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 130.576 -40.737 0.598 -6.031 4.341 49.62
Hunt & Reffert 2024 130.588 -40.735 0.607 -5.946 4.166 47.361
Celli et al. 2024 130.571 -40.737 – – – –
Cavallo et al. 2024 130.638 -40.712 0.621 – – –
Hunt & Reffert 2023 130.588 -40.735 0.607 -5.946 4.166 47.361
Cantat-Gaudin et al. 2020 130.571 -40.737 0.613 -5.998 4.44 –
Cantat-Gaudin & Anders 2020 130.571 -40.737 0.613 -5.998 4.44 –
Cantat-Gaudin et al. 2018 130.571 -40.737 0.613 -5.998 4.44 –

💡 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
Hunt & Reffert 2024 – – – – – 173* – –
Celli et al. 2024 – – – 10 – 120 – –
Cavallo et al. 2024 2.07 3.18 – 37 0.240 – – –
Hunt & Reffert 2023 1.53 2.78 2.64 211 – – – –
Cantat-Gaudin et al. 2020 1.58 3.26 – 10 – – – –
Cantat-Gaudin & Anders 2020 1.56 – – – – – – –
Cantat-Gaudin et al. 2018 1.56 – – – – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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