IRAS 02245+6115

0.02 UTI

0.0

C_N

0.23

C_dens

0.12

C_C3

0.0

C_lit

0.28

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 1.2 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.23 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

IRAS 02245+6115 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 23 years.

⚠️ Warning: This is possibly a duplicate object, which shares a significant 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=0.28) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close

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

Data

🔍 Search references for IRAS 02245+6115 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	37.255	61.498	0.436	-1.199	-0.192	-29.807
Lada & Lada	2003	37.09	61.475	–	–	–	–

💡 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–	2.4	–	–	–	–	77	–	–
Lada & Lada	2003	2.40	–	–	–	–	77	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
AFGL333	72.0	37.29	61.48	0.44	-1.17	-0.17	-29.81	0.14
IC1805-West	4.0	37.27	61.55	0.41	-0.96	-0.59	–	0.14

💡 Note: The % column shows the percentage of members that IRAS 02245+6115 shares with each listed object.

Visualization

ℹ️