UBC 1361

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0.00 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.31 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 1361 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Massive 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 – 106.135 -11.256 0.147 -0.443 1.043 57.048
Hu & Soubiran 2025 106.143 -11.265 – – – –
Hunt & Reffert 2024 106.137 -11.252 0.15 -0.455 1.034 57.068
Cavallo et al. 2024 106.143 -11.265 0.148 – – –
Hunt & Reffert 2023 106.137 -11.252 0.15 -0.455 1.034 57.068
Castro-Ginard et al. 2022 106.14 -11.26 0.14 -0.45 1.04 –

💡 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
Hu & Soubiran 2025 – – – – -0.510* – – –
Hunt & Reffert 2024 – – – – – 1867* – –
Cavallo et al. 2024 5.55 2.30 – 891 -0.120 – – –
Hunt & Reffert 2023 5.92 1.97 1.93 1009 – – – –
Castro-Ginard et al. 2022 9.62 1.77 – 526 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Juchert 7 100.0 106.14 -11.26 0.16 -0.45 1.05 62.09 0.51

💡 Note: The % column shows the percentage of members that UBC 1361 shares with each listed object.

Visualization

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