IRAS 02232+6138

(MWSC 192)

0.01 UTI

0.7

C_N

1.0

C_dens

1.0

C_C3

0.31

C_lit

0.01

C_dup

C3 classification AA

Number of members (P>50%) 91

Radius (P>50% members) 1.9 [arcmin]

C_N 0.7 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.31 Poorly studied
C_dup 0.01 Very likely duplicate

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

Overview

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IRAS 02232+6138 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High extinction Very young

Data

🔍 Search references for IRAS 02232+6138 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	–	36.645	62.0	0.484	-0.685	-0.131	-24.583
Just et al.	2023	36.63	61.986	–	–	–	–
Loktin & Popova	2017	36.645	61.99	–	1.789	0.328	–
Kharchenko et al.	2016	36.63	61.986	–	–	–	–
Kharchenko et al.	2013	36.642	61.988	–	-0.85	1.3	-47.1
Kharchenko et al.	2012	36.642	61.988	–	1.17	0.59	–

💡 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	–	–	–	7	–	152	–	–
Loktin & Popova	2017	2.00	2.86	–	32	–	–	–	–
Kharchenko et al.	2016	1.83	3.68	–	7	–	–	–	–
Kharchenko et al.	2013	1.83	3.68	–	7	–	–	–	–
Kharchenko et al.	2012	1.70	3.10	–	711	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 19	98.9	36.65	62.0	0.48	-0.7	-0.12	-27.12	0.55
CWNU 3691	56.0	36.65	62.0	0.47	-0.69	-0.06	-21.84	0.02

💡 Note: The % column shows the percentage of members that IRAS 02232+6138 shares with each listed object.

Visualization

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