IRAS 06567-0355

(MWSC 1047)

0.05 UTI

0.0

C_N

0.18

C_dens

0.25

C_C3

0.0

C_lit

0.56

C_dup

C3 classification CC

Number of members (P>50%) 21

Radius (P>50% members) 5.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.56 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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IRAS 06567-0355 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* 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.

(*): The parallax distance estimate (~2.78 kpc) differs significantly from the median photometric distance (~1.94 kpc).

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.

Relatively close Moderate extinction Young

Data

🔍 Search references for IRAS 06567-0355 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	–	104.833	-3.939	0.36	-1.77	0.764	–
Just et al.	2023	104.813	-3.969	–	–	–	–
Kharchenko et al.	2016	104.813	-3.969	–	–	–	–
Kharchenko et al.	2013	104.82	-3.97	–	0.41	4.36	39.6

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	22	–	224	–	–
Kharchenko et al.	2016	1.94	2.00	–	22	–	–	–	–
Kharchenko et al.	2013	1.94	2.00	–	22	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Ivanov 9	44.0	104.94	-4.06	0.31	-1.77	0.8	–	0.14

💡 Note: The % column shows the percentage of members that IRAS 06567-0355 shares with each listed object.

Visualization

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