UBC 1513

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0.58 UTI
0.4
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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UBC 1513 is a poorly populated, very dense object of very high 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, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a small percentage of members with a later reported entry. See table with shared members information.

Distant 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 – 182.055 -61.887 0.309 -5.357 0.097 -11.112
Hunt & Reffert 2024 182.013 -61.884 0.302 -5.374 0.089 -11.107
Cavallo et al. 2024 182.061 -61.891 0.303 – – –
Hunt & Reffert 2023 182.013 -61.884 0.302 -5.374 0.089 -11.107
Castro-Ginard et al. 2022 182.08 -61.88 0.31 -5.37 0.08 –

💡 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 – – – – – 347* – –
Cavallo et al. 2024 2.57 1.54 – 257 0.140 – – –
Hunt & Reffert 2023 3.27 1.70 1.47 74 – – – –
Castro-Ginard et al. 2022 3.25 1.19 – 74 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 9456 25.0 182.02 -61.92 0.29 -5.46 0.16 -11.11 0.04

💡 Note: The % column shows the percentage of members that UBC 1513 shares with each listed object.

Visualization

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