IRAS 02570+6028

0.21 UTI

0.26

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.65

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 7.6 [N/pc²]

C3 classification BC

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.65 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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IRAS 02570+6028 is a poorly 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 likely a unique object, which shares a moderate 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 02570+6028 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–	45.18	60.629	0.424	-0.11	0.065	-30.542
Lada & Lada	2003	45.253	60.672	–	–	–	–

💡 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	–	–	–	–	50	–	–
Lada & Lada	2003	2.40	–	–	–	–	50	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
AFGL 4029	34.6	45.21	60.54	0.44	-0.13	0.03	-30.61	0.14
SAI 24	34.6	44.83	60.57	0.45	-0.23	0.07	-49.28	0.91
IRAS 02575+6017	26.9	45.26	60.52	0.42	-0.06	-0.09	-30.61	0.36

💡 Note: The % column shows the percentage of members that IRAS 02570+6028 shares with each listed object.

Visualization

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