IRAS 06562-0337 Cl

0.05 UTI

0.0

C_N

0.1

C_dens

0.12

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 23

Core radius and density 2.2 [pc], 0.5 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.1 Very loose
C_C3 0.12 Very 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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IRAS 06562-0337 Cl is a sparse, very loose object of very low 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 23 years.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

No fundamental parameters

Bica et al. (2003)
Classified as infrared cluster (IRC).

Data

🔍 Search references for IRAS 06562-0337 Cl 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–	104.7	-3.682	0.245	-0.809	0.988	78.223
Bica et al.	2003	104.691	-3.678	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IRAS 06562-0337	28.0	104.69	-3.68	0.18	-0.66	0.72	–	0.05

💡 Note: The % column shows the percentage of members that IRAS 06562-0337 Cl shares with each listed object.

Visualization

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