DBSB 39

(MWSC 1665)

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0.45 UTI
0.38
CN
0.39
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.39 Loose
  • CC3 0.75 High quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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DBSB 39 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.77 kpc) differs significantly from the median photometric distance (~2.12 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 141.149 -53.108 0.36 -4.971 3.844 –
Hunt & Reffert 2024 141.126 -53.126 0.358 -4.96 3.843 19.786
Cavallo et al. 2024 141.142 -53.085 0.361 – – –
Hunt & Reffert 2023 141.126 -53.126 0.358 -4.96 3.843 19.786
Just et al. 2023 141.098 -53.132 – – – –
Kharchenko et al. 2016 141.098 -53.132 – – – –
Kharchenko et al. 2013 141.103 -53.136 – -0.73 7.19 –

💡 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 – – – – – 828* – –
Cavallo et al. 2024 2.39 1.24 – 34 0.490 – – –
Hunt & Reffert 2023 2.50 1.60 2.15 18 – – – –
Just et al. 2023 – – – 25 – 18 – –
Kharchenko et al. 2016 1.86 2.39 – 25 – – – –
Kharchenko et al. 2013 1.86 2.39 – 25 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 489 97.4 141.15 -53.08 0.35 -4.95 3.82 – 0.18

💡 Note: The % column shows the percentage of members that DBSB 39 shares with each listed object.

Visualization

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