IRAS 02232+6138

(MWSC 192)

0.68 UTI

0.7

C_N

1.0

C_dens

1.0

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 91

Stellar density (N₅₀/rad) 69.9 [N/pc²]

C3 classification AA

C_N 0.7 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 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.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close High extinction Very young

Lada & Lada (2003)
Embedded cluster within ∼2 Kpc of the Sun.

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	99999–	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	–
Lada & Lada	2003	36.767	61.873	–	–	–	–

💡 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–	1.83	3.39	–	7	–	141	–	–
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	–	–	–	–
Lada & Lada	2003	2.40	–	–	–	–	130	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
SAI 19	98.9	36.65	62.0	0.48	-0.7	-0.12	-27.12	0.1
CWNU 3691	56.0	36.65	62.0	0.47	-0.69	-0.06	-21.84	0.02
W3IRS5	4.4	36.41	62.09	0.46	-1.0	-0.53	30.96	0.19

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

Visualization

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