MCM 88

(MCM2005b 88)

0.31 UTI

0.45

C_N

0.85

C_dens

0.25

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 4.2 [N/pc²]

C3 classification CC

C_N 0.45 Poorly populated
C_dens 0.85 Dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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MCM 88 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 13 years.

(*): The parallax distance estimate (~2.33 kpc) differs significantly from the median photometric distance (~1.61 kpc).

Relatively close

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of emission related to PAH or warm dust.

Mercer et al. (2005)
Cluster of stars. Associated with mid-IR extended emission.

Data

🔍 Search references for MCM 88 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–	256.15	-40.795	0.429	-1.702	-1.713	-5.492
Morales et al.	2013	256.129	-40.775	–	–	–	–
Mercer et al.	2005	256.128	-40.775	–	–	–	–

💡 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–	1.61	–	–	–	–	–	–	–
Morales et al.	2013	1.61	–	–	–	–	–	–	–

Visualization

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