HXHWL 42

(H21OC 42)

0.37 UTI

0.26

C_N

0.57

C_dens

0.38

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 26

Radius (P>50% members) 9.2 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.57 Moderately dense
C_C3 0.38 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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HXHWL 42 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for HXHWL 42 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	–	122.335	-35.598	0.888	-4.735	3.007	18.151
Hunt & Reffert	2024	122.322	-35.659	0.891	-4.765	2.993	11.784
Cavallo et al.	2024	122.367	-35.599	0.892	–	–	–
Hunt & Reffert	2023	122.322	-35.659	0.891	-4.765	2.993	11.784
He et al.	2022	122.244	-35.542	0.874	-4.669	3.011	–
He et al.	2021	122.332	-35.568	0.86	-4.78	2.97	–

💡 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
Hunt & Reffert	2024	–	–	–	–	–	156*	–	–
Cavallo et al.	2024	1.13	0.62	–	219	0.320	–	–	–
Hunt & Reffert	2023	1.06	0.43	0.81	137	–	–	–	–
He et al.	2022	–	0.85	–	63	–	–	–	–
He et al.	2021	1.20	0.84	–	91	0.537	–	–	–

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

Visualization

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