UBC 265

0.23 UTI

0.78

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.45

C_dup

C3 classification AB

Number of members (P>50%) 185

Radius (P>50% members) 8.3 [arcmin]

C_N 0.78 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.45 Possibly duplicate

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

Overview

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UBC 265 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 6 years.

⚠️ 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.

No fundamental parameters

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

🔍 Search references for UBC 265 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	–	167.71	-56.81	0.837	-7.452	0.705	1.164
Castro-Ginard et al.	2020	167.699	-56.819	0.81	-7.463	0.669	–

💡 Note: The UCC values are estimated from its identified members.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14043	62.7	167.72	-56.81	0.85	-7.44	0.72	-0.88	0.0
FoF 2238	55.1	167.72	-56.81	0.85	-7.45	0.71	0.54	0.76

💡 Note: The % column shows the percentage of members that UBC 265 shares with each listed object.

Visualization

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