IRAS 05100+3723

0.43 UTI

0.26

C_N

1.0

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 26

Radius (P>50% members) 2.1 [arcmin]

C_N 0.26 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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IRAS 05100+3723 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for IRAS 05100+3723 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	–	78.368	37.428	0.291	0.021	-1.468	–
Zhang et al.	2024	78.358	37.441	–	–	–	–
Hunt & Reffert	2024	78.358	37.441	0.284	0.006	-1.464	-6.35
Cavallo et al.	2024	78.443	37.402	0.283	–	–	–
Hunt & Reffert	2023	78.358	37.441	0.284	0.006	-1.464	-6.35

💡 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]	Bfr	BSS
Zhang et al.	2024	–	–	–	–	-0.140*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	576*	–	–
Cavallo et al.	2024	3.18	2.67	–	437	0.140	–	–	–
Hunt & Reffert	2023	3.13	2.56	2.26	237	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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