IRAS 02407+6047

0.04 UTI

0.31

C_N

0.08

C_dens

0.12

C_C3

0.0

C_lit

0.42

C_dup

N₅₀ (P>50% members) 31

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification DC

C_N 0.31 Poorly populated
C_dens 0.08 Very loose
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.42 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 02407+6047 is a poorly populated, 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 low-mass 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.

(*): The parallax distance estimate (~4.84 kpc) differs significantly from the median photometric distance (~2.40 kpc).

Relatively close Low mass

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

Data

🔍 Search references for IRAS 02407+6047 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–	41.084	61.042	0.206	-0.467	-0.429	-35.723
Lada & Lada	2003	41.157	60.998	–	–	–	–

💡 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	–	–	–	–	32	–	–
Lada & Lada	2003	2.40	–	–	–	–	32	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Majaess 30	58.1	41.07	61.02	0.17	-0.44	-0.42	–	0.03

💡 Note: The % column shows the percentage of members that IRAS 02407+6047 shares with each listed object.

Visualization

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