IRAS 02575+6017

0.36 UTI

0.68

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.87

C_dup

N₅₀ (P>50% members) 85

Stellar density (N₅₀/rad) 11.3 [N/pc²]

C3 classification BC

C_N 0.68 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.87 Very likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 02575+6017 is a moderately populated, very dense object of 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.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close

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

Data

🔍 Search references for IRAS 02575+6017 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–	45.258	60.518	0.424	-0.058	-0.093	-30.615
Lada & Lada	2003	45.372	60.487	–	–	–	–

💡 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	–	–	–	–	150	–	–
Lada & Lada	2003	2.40	–	–	–	–	150	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
AFGL 4029	28.2	45.21	60.54	0.44	-0.13	0.03	-30.61	0.14
SAI 24	12.9	44.83	60.57	0.45	-0.23	0.07	-49.28	0.91
IRAS 02570+6028	8.2	45.18	60.63	0.42	-0.11	0.06	-30.54	0.21
Collinder 34	1.2	44.83	60.57	0.44	-0.35	0.04	-55.55	0.18

💡 Note: The % column shows the percentage of members that IRAS 02575+6017 shares with each listed object.

Visualization

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