IRAS 06562-0337

(MWSC 1041)

0.04 UTI

0.0

C_N

0.11

C_dens

0.12

C_C3

0.03

C_lit

0.72

C_dup

N_m (P>50%) 19

Core radius and density 1.7 [pc], 0.6 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.11 Very loose
C_C3 0.12 Very low quality
C_lit 0.03 Rarely studied
C_dup 0.72 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 06562-0337 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

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.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=0.72) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very distant Moderate extinction Young

Data

🔍 Search references for IRAS 06562-0337 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–	104.686	-3.681	0.182	-0.658	0.721	–
Just et al.	2023	104.676	-3.683	–	–	–	–
Kharchenko et al.	2016	104.676	-3.683	–	–	–	–
Kharchenko et al.	2013	104.683	-3.685	–	0.51	2.57	53.0

💡 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–	6.09	2.96	–	50	–	522	–	–
Just et al.	2023	–	–	–	50	–	522	–	–
Kharchenko et al.	2016	6.09	2.96	–	50	–	–	–	–
Kharchenko et al.	2013	6.09	2.96	–	50	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IRAS 06562-0337 Cl	28.0	104.7	-3.68	0.24	-0.81	0.99	78.22	0.04

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

Visualization

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