DBSB 19

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0.42 UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.83
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.83 Very likely unique

Overview

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DBSB 19 is a rich, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Old

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 – 128.892 -40.622 1.056 -5.861 3.321 23.993
Hunt & Reffert 2024 128.899 -40.61 1.061 -5.854 3.321 24.863
Cavallo et al. 2024 128.929 -40.605 1.059 – – –
Hunt & Reffert 2023 128.899 -40.61 1.061 -5.854 3.321 24.863

💡 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 – – – – – 221* – –
Cavallo et al. 2024 1.73 1.39 – 4467 0.390 – – –
Hunt & Reffert 2023 0.90 3.00 2.48 5 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0469 17.1 128.9 -40.62 1.05 -5.86 3.33 30.14 0.42

💡 Note: The % column shows the percentage of members that DBSB 19 shares with each listed object.

Visualization

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