UBC 1417

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0.41 UTI
0.36
CN
0.44
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.4 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1417 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
Distant Low extinction Near-solar metallicity Intermediate age

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 – 121.262 -30.696 0.245 -2.616 3.498 132.893
Hunt & Reffert 2024 121.268 -30.697 0.245 -2.615 3.508 –
Cavallo et al. 2024 121.257 -30.71 0.246 – – –
Hunt & Reffert 2023 121.268 -30.697 0.245 -2.615 3.508 –
Castro-Ginard et al. 2022 121.24 -30.7 0.26 -2.63 3.51 –

💡 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 – – – – – 250* – –
Cavallo et al. 2024 3.63 1.35 – 38 -0.270 – – –
Hunt & Reffert 2023 4.01 0.54 1.29 366 – – – –
Castro-Ginard et al. 2022 4.52 0.77 – 315 – – – –

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

Visualization

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