IRAS 02048+5957

0.04 UTI

0.0

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.12

C_dup

N₅₀ (P>50% members) 20

Stellar density (N₅₀/rad) 8.8 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 02048+5957 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near 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 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 Low mass

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

Data

🔍 Search references for IRAS 02048+5957 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–	31.91	60.252	0.347	-0.795	-0.494	20.458
Lada & Lada	2003	32.112	60.196	–	–	–	–

💡 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	–	–	–	–	37	–	–
Lada & Lada	2003	2.40	–	–	–	–	37	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Riddle 4	88.0	31.86	60.26	0.35	-0.79	-0.49	-44.58	0.91

💡 Note: The % column shows the percentage of members that IRAS 02048+5957 shares with each listed object.

Visualization

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