UBC 161

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0.00 UTI
0.74
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.74 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

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UBC 161 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, intermediate-age cluster (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.

Relatively close Moderate extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 319.099 57.462 0.711 -3.092 -4.486 -19.99
Hunt & Reffert 2024 319.129 57.464 0.712 -3.079 -4.47 -22.51
Cavallo et al. 2024 319.114 57.461 0.713 – – –
Hunt & Reffert 2023 319.129 57.464 0.712 -3.079 -4.47 -22.51
Castro-Ginard et al. 2020 319.082 57.447 0.702 -3.123 -4.427 –

💡 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 – – – – – 643* – –
Cavallo et al. 2024 1.64 1.77 – 224 0.660 – – –
Hunt & Reffert 2023 1.34 1.71 2.07 144 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2000 100.0 319.09 57.46 0.71 -3.09 -4.48 -21.36 0.65

💡 Note: The % column shows the percentage of members that UBC 161 shares with each listed object.

Visualization

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