MCM 50

0.22 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.43

C_dup

N₅₀ (P>50% members) 122

Stellar density (N₅₀/rad) 32.9 [N/pc²]

C3 classification AB

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.43 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MCM 50 is a rich, very dense object of high 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 21 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

Data

🔍 Search references for MCM 50 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–	214.82	-61.431	0.574	-3.252	-3.095	-41.325
Mercer et al.	2005	214.913	-61.422	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Loden 1256	56.6	214.77	-61.43	0.58	-3.28	-3.11	-55.63	0.66
OC 0608	20.5	214.85	-61.43	0.59	-3.19	-3.14	-55.63	0.0

💡 Note: The % column shows the percentage of members that MCM 50 shares with each listed object.

Visualization

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