UBC 1570

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0.50 UTI
0.26
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.1 [arcmin]
  • CN 0.26 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 1570 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate 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 – 298.14 32.547 0.396 -2.404 -5.386 -2.321
Hunt & Reffert 2024 298.145 32.558 0.401 -2.377 -5.345 -2.338
Cavallo et al. 2024 298.125 32.559 0.4 – – –
Hunt & Reffert 2023 298.145 32.558 0.401 -2.377 -5.345 -2.338
Castro-Ginard et al. 2022 298.12 32.54 0.4 -2.41 -5.39 -2.46

💡 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 – – – – – 210* – –
Cavallo et al. 2024 1.94 1.84 – 316 0.100 – – –
Hunt & Reffert 2023 2.34 1.82 1.58 168 – – – –
Castro-Ginard et al. 2022 2.76 1.30 – 291 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 11583 100.0 298.14 32.54 0.41 -2.4 -5.38 -2.32 0.13
CWNU 517 92.3 298.13 32.55 0.4 -2.4 -5.39 -2.32 0.03

💡 Note: The % column shows the percentage of members that UBC 1570 shares with each listed object.

Visualization

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