UBC 1517

0.22 UTI

0.75

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.4

C_dup

C3 classification AA

Number of members (P>50%) 110

Radius (P>50% members) 2.4 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

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

Overview

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UBC 1517 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for UBC 1517 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	193.77	-61.055	0.315	-5.23	-0.347	-5.798
Castro-Ginard et al.	2022	193.79	-61.06	0.31	-5.23	-0.36	-14.71

💡 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
Castro-Ginard et al.	2022	3.50	1.39	–	149	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 231	89.1	193.77	-61.05	0.32	-5.23	-0.35	13.85	0.01
ASCC 72	60.0	193.77	-61.04	0.32	-5.23	-0.34	-4.35	0.78

💡 Note: The % column shows the percentage of members that UBC 1517 shares with each listed object.

Visualization

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