UBC 1595

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0.52 UTI
0.37
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.1 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1595 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close 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.
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 – 289.961 -1.895 1.063 -0.779 -2.135 4.963
Hunt & Reffert 2024 289.951 -1.872 1.069 -0.797 -2.153 -20.105
Cavallo et al. 2024 289.936 -1.934 1.069 – – –
Hunt & Reffert 2023 289.951 -1.872 1.069 -0.797 -2.153 -20.105
Castro-Ginard et al. 2022 289.95 -1.87 1.07 -0.78 -2.12 –

💡 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 – – – – – 130* – –
Cavallo et al. 2024 1.04 2.33 – 32 0.080 – – –
Hunt & Reffert 2023 0.89 1.73 0.90 33 – – – –
Castro-Ginard et al. 2022 1.03 2.13 – 126 – – – –

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

Visualization

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