AFGL 4029

0.14 UTI

0.3

C_N

0.9

C_dens

0.12

C_C3

0.0

C_lit

0.53

C_dup

N₅₀ (P>50% members) 30

Stellar density (N₅₀/rad) 4.5 [N/pc²]

C3 classification DC

C_N 0.3 Poorly populated
C_dens 0.9 Very dense
C_C3 0.12 Very low quality
C_lit 0.0 Rarely studied
C_dup 0.53 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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AFGL 4029 is a poorly populated, very dense 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.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a large 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 AFGL 4029 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–	45.205	60.543	0.44	-0.128	0.034	-30.615
Lada & Lada	2003	45.385	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–	2.2	–	–	–	–	140	–	–
Lada & Lada	2003	2.20	–	–	–	–	140	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
IRAS 02575+6017	80.0	45.26	60.52	0.42	-0.06	-0.09	-30.61	0.36
SAI 24	46.7	44.83	60.57	0.45	-0.23	0.07	-49.28	0.91
IRAS 02570+6028	30.0	45.18	60.63	0.42	-0.11	0.06	-30.54	0.21
Collinder 34	13.3	44.83	60.57	0.44	-0.35	0.04	-55.55	0.18

💡 Note: The % column shows the percentage of members that AFGL 4029 shares with each listed object.

Visualization

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