UBC 1013

0.10 UTI

0.43

C_N

0.77

C_dens

1.0

C_C3

0.0

C_lit

0.23

C_dup

N₅₀ (P>50% members) 43

Stellar density (N₅₀/rad) 3.8 [N/pc²]

C3 classification AA

C_N 0.43 Poorly populated
C_dens 0.77 Dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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UBC 1013 is a poorly populated, dense object of very 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 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.

Relatively close Moderate extinction Very young

Data

🔍 Search references for UBC 1013 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	99999–	273.113	-15.375	0.582	-0.234	-1.744	32.924
Castro-Ginard et al.	2022	273.13	-15.33	0.58	-0.24	-1.76	–

💡 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]	B_frac	BSS
UCC	99999–	1.84	1.2	–	11	–	–	–	–
Castro-Ginard et al.	2022	1.84	1.20	–	11	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 13990	79.1	273.11	-15.38	0.59	-0.25	-1.77	27.73	0.01
HXHWL 66	76.7	273.12	-15.38	0.58	-0.24	-1.74	2.21	0.51

💡 Note: The % column shows the percentage of members that UBC 1013 shares with each listed object.

Visualization

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