UBC 514

0.35 UTI

0.0

C_N

0.12

C_dens

0.75

C_C3

0.44

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 24

Radius (P>50% members) 11.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.12 Very loose
C_C3 0.75 High quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

ℹ️

UBC 514 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Relatively close Low extinction Near-solar metallicity Old

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for UBC 514 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	158.633	-73.312	0.529	-6.882	1.13	-23.083
Li et al.	2025	158.561	-73.324	0.504	-6.926	1.087	–
Hu & Soubiran	2025	158.503	-73.261	–	–	–	–
Cavallo et al.	2024	158.503	-73.261	0.531	–	–	–
Hunt & Reffert	2023	158.689	-73.087	0.531	-6.886	1.133	-32.184
Almeida et al.	2023	158.528	-73.257	–	–	–	–
Dias et al.	2021	158.515	-73.289	0.508	-6.876	1.12	–
Cantat-Gaudin et al.	2020	158.561	-73.324	0.504	-6.926	1.087	–

💡 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
Li et al.	2025	1.62	0.40	–	3491	-0.151	–	–	–
Hu & Soubiran	2025	–	–	–	–	-0.260*	–	–	–
Cavallo et al.	2024	1.90	0.58	–	1778	0.160	–	–	–
Hunt & Reffert	2023	1.81	0.36	0.51	1452	–	–	–	–
Almeida et al.	2023	1.81	0.55	–	3126	-0.210	268*	0.78	–
Dias et al.	2021	1.89	0.38	–	3192	0.072	–	–	–
Cantat-Gaudin et al.	2020	1.85	0.73	–	2239	–	–	–	–

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

Visualization

ℹ️

1 2 3