DBSB 104

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0.55 UTI
0.0
CN
1.0
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 5.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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DBSB 104 is a sparse, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very 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 – 255.985 -51.103 0.897 -0.492 -2.633 -17.833
Hunt & Reffert 2024 255.97 -51.092 0.91 -0.505 -2.622 -15.078
Celli et al. 2024 255.997 -51.088 – – – –
Cavallo et al. 2024 255.918 -51.1 0.91 – – –
Hunt & Reffert 2023 255.97 -51.092 0.91 -0.505 -2.622 -15.078
He et al. 2022 255.957 -51.074 0.917 -0.541 -2.547 –
Cantat-Gaudin et al. 2020 255.997 -51.088 0.908 -0.443 -2.692 –
Cantat-Gaudin & Anders 2020 255.997 -51.088 0.908 -0.443 -2.692 –
Cantat-Gaudin et al. 2018 255.997 -51.088 0.908 -0.443 -2.692 –

💡 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 – – – – – 51* – –
Celli et al. 2024 – – – 27 – 67 – –
Cavallo et al. 2024 1.02 1.31 – 4 0.030 – – –
Hunt & Reffert 2023 1.04 0.89 1.33 5 – – – –
He et al. 2022 – 1.60 – 5 – – – –
Cantat-Gaudin et al. 2020 1.08 0.88 – 27 – – – –
Cantat-Gaudin & Anders 2020 1.07 – – – – – – –
Cantat-Gaudin et al. 2018 1.07 – – – – – – –

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

Visualization

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