UBC 1432

0.09 UTI

0.41

C_N

0.56

C_dens

1.0

C_C3

0.0

C_lit

0.22

C_dup

C3 classification AA

Number of members (P>50%) 41

Radius (P>50% members) 2.0 [arcmin]

C_N 0.41 Poorly populated
C_dens 0.56 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.22 Likely duplicate

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

Overview

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UBC 1432 is a poorly populated, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is 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 Very young

Data

🔍 Search references for UBC 1432 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	–	124.82	-34.479	0.152	-2.589	3.235	–
Castro-Ginard et al.	2022	124.76	-34.49	0.16	-2.59	3.24	–

💡 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	7.82	1.45	–	14	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ruprecht 59	78.0	124.82	-34.48	0.15	-2.59	3.24	–	0.52

💡 Note: The % column shows the percentage of members that UBC 1432 shares with each listed object.

Visualization

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