MCM 36

(MCM2005b 36)

0.13 UTI

0.0

C_N

0.03

C_dens

0.62

C_C3

0.0

C_lit

0.96

C_dup

N₅₀ (P>50% members) 19

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification AC

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.96 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

MCM 36 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate 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 13 years.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Morales et al. (2013)
Classified as morphological type 'EC1' (deeply embedded cluster). Morphological flag: cluster fully embedded, presence of an IR bubble.

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

Data

🔍 Search references for MCM 36 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	198.362	-63.036	0.203	-6.769	-0.625	-35.166
Morales et al.	2013	198.267	-63.006	–	–	–	–
Mercer et al.	2005	198.268	-63.006	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
DBSB 134	4.0	198.38	-62.72	0.17	-6.99	-0.6	-31.82	0.13

💡 Note: The % column shows the percentage of members that MCM 36 shares with each listed object.

Visualization

ℹ️