UBC 242

0.28 UTI

0.8

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.58

C_dup

N₅₀ (P>50% members) 242

Stellar density (N₅₀/rad) 9.6 [N/pc²]

C3 classification AC

C_N 0.8 Rich
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.58 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UBC 242 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near 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.

Note: This is likely a unique object, which shares a moderate 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 242 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–	127.441	-41.322	0.725	-1.778	1.109	-1.423
Castro-Ginard et al.	2020	127.479	-41.349	0.72	-1.791	1.078	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 2220	42.1	127.44	-41.33	0.73	-1.77	1.11	-6.24	0.75
CWWDL 14141	12.8	127.61	-41.38	0.73	-1.76	1.12	-1.55	0.0

💡 Note: The % column shows the percentage of members that UBC 242 shares with each listed object.

Visualization

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