Cmg 1050

0.06 UTI

0.0

C_N

0.08

C_dens

0.5

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 24

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

Cmg 1050 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 7 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

Data

🔍 Search references for Cmg 1050 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	114.864	-33.65	0.264	-2.243	3.033	–
Bica et al.	2019	114.848	-33.777	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Bochum 15	48.0	115.08	-33.57	0.26	-2.24	3.04	–	0.3
CWNU 3351	48.0	115.07	-33.57	0.26	-2.25	3.04	–	0.05

💡 Note: The % column shows the percentage of members that Cmg 1050 shares with each listed object.

Visualization

ℹ️