UBC 1527

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0.49 UTI
0.47
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.5 [arcmin]
  • CN 0.47 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1527 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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 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 – 217.687 -60.397 0.43 -4.895 -3.058 -85.855
Hunt & Reffert 2024 217.728 -60.398 0.423 -4.907 -3.04 -47.408
Cavallo et al. 2024 217.606 -60.384 0.424 – – –
Hunt & Reffert 2023 217.728 -60.398 0.423 -4.907 -3.04 -47.408
Castro-Ginard et al. 2022 217.7 -60.4 0.44 -4.9 -3.06 –

💡 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 – – – – – 572* – –
Cavallo et al. 2024 1.87 2.13 – 21 0.020 – – –
Hunt & Reffert 2023 2.16 2.44 2.00 16 – – – –
Castro-Ginard et al. 2022 2.18 1.98 – 9 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 31 85.1 217.71 -60.39 0.43 -4.88 -3.06 -85.85 0.06

💡 Note: The % column shows the percentage of members that UBC 1527 shares with each listed object.

Visualization

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